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204
Jun 21, 2010
06/10
by
NON
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Cost effectiveness of improved landing capability on airline operations
Topics: ABSORPTION SPECTRA, ATMOSPHERIC DIFFUSION, STELLAR SPECTROPHOTOMETRY, POINT SOURCES, SPECTROSCOPIC...
305
305
May 29, 2011
05/11
by
Luckring, J. M.; Ghee, T. A
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An advanced diamond-wing configuration was tested at low speeds in the National Transonic Facility (NTF) in air at chord Reynolds numbers from 4.4 million (typical wind-tunnel conditions) to 24 million (nominal flight value). Extensive variations on high-lift rigging were explored as part of a broad multinational program. The analysis for this study is focused on the cruise and landing settings of the wing high-lift systems. Three flow domains were identified from the data and provide a context...
Topics: ELECTROPHOTOMETRY, ORION CONSTELLATION, UBV SPECTRA, BRIGHTNESS, ECLIPSES, ESTIMATES, STELLAR...
451
451
Aug 1, 2010
08/10
by
Litt, Jonathan S.; Smith, Ira C
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Tuning maps are an aid in the controller tuning process because they provide a convenient way for the plant operator to determine the consequences of adjusting different controller parameters. In this application the maps provide a graphical representation of the effect of varying the gains in the state feedback matrix on startup and load disturbance transients for a three capacity process. Nominally, the three tank system, represented in diagonal form, has a Proportional-Integral control on...
Topics: ASTRONOMICAL CATALOGS, COMPUTER COMPATIBLE TAPES, STELLAR SPECTROPHOTOMETRY, DIGITAL DATA, TABLES...
Transformations are found for converting the b-y color excesses for Cepheids given by Williams (1966) and Kelsall (1971) into B-V excesses. The combination of these results with the E(B-V)'s determined by Sandage and Tammann (1971) gives precise data for eighty-eight galactic Cepheids. The period-color and period-color-(amplitude defect) relationships, that are germane to the LogP intervals 0.4 to 1.4 and 0.4 to 1.3, respectively, are found.
Topics: NASA Technical Reports Server (NTRS), CEPHEID VARIABLES, STELLAR SPECTROPHOTOMETRY, COLOR, LIGHT...
215
215
Jul 6, 2010
07/10
by
Wands, R. C
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Preventive measures of occupational medicine and industrial hygiene are coordinated to identify toxicities of industrial products and safety standards in manned space flight applications. Emphasized is the off-gassing of construction materials in spacecraft with the resulting contamination of the cabin atmosphere and the establishment of criteria for the quality of drinking water for astronauts during Gemini and Apollo programs.
Topics: SALYUT SPACE STATION, SPACEBORNE TELESCOPES, STELLAR SPECTROPHOTOMETRY, CENTAURUS CONSTELLATION,...
Absolute spectral energy distributions for the large redshift quasars OQ 172 and OH 471 are discussed along with similar data for two other quasars 4C05.34 and PHL 957. Assuming cosmological redshifts, OQ 172 and OH 471 are not as luminous as PHL 957. If these quasars are basically similar and if radiative processes dominate, the strength of Ly alpha and the behavior of the continuum at the Lyman limit strongly suggest that these objects consist of a central ionizing source surrounded by...
Topics: NASA Technical Reports Server (NTRS), PHOTOELECTRICITY, QUASARS, STELLAR SPECTROPHOTOMETRY,...
Photometric data from the Wisconsin Experiment package on OAO-2 were obtained for six Beta Cephei variable stars. The data were reduced in accordance with the OAO 2/Wisconsin Experiment Package Photometer Users Guide. For delta Cet and gamma Peg, there were enough data points to form reliable composite light curves at seven or eight ultraviolet wavelengths. The light curves are well represented by sine waves in phase with the blue light curve for each star. The amplitude of the light variation...
Topics: NASA Technical Reports Server (NTRS), OAO 2, STELLAR SPECTROPHOTOMETRY, VARIABLE STARS, LIGHT...
Spectral observations of the stars alpha CMa, gamma Ori, kappa Ori, and alpha Leo have been obtained in the range 1150 to 4000 Angstroms, using rocket borne spectrometers. The payloads have a 13-inch diameter telescope, a rotatable concave diffraction grating, and three pulse counting photomultiplier photometers. The laboratory standards used as photometric references derive their primary calibration directly or indirectly from the National Bureau of Standards. An error range of up to + or - 10...
Topics: NASA Technical Reports Server (NTRS), ASTRONOMY, STELLAR SPECTROPHOTOMETRY, ULTRAVIOLET...
Observations of celestial phenomena need to be calibrated, to be related, to some measurable quantity. There continues to be a long-term need for accurate photometric standard stars, those with known intensities and colors, so that brightness and color measurements made of various celestial phenomena by different observers can be integrated and compared with one another. Toward this end, the author has been emphasizing data collection in recent years for stars of 'intermediate' brightness,...
Topics: NASA Technical Reports Server (NTRS), CALIBRATING, CELESTIAL BODIES, DATA ACQUISITION, STELLAR...
New observations of the Crab Nebula by OAO 2 stellar photometers are reported. Processed image data of the Crab give the logarithm of the integrated relative intensity per wavelength interval, corrected for sky background, and the rms error from 11 passbands in the ultraviolet range. The data are converted to logarithms of flux density per frequency interval and plotted on logarithmic scales with corrections for interstellar extinction.
Topics: NASA Technical Reports Server (NTRS), CRAB NEBULA, OAO 2, ULTRAVIOLET PHOTOMETRY, SATELLITE-BORNE...
A progress report on the IRAF stellar photometry package DIGIPHOT, with emphasis on algorithm enhancements and photometry catalog processing tools is presented. The IRAF implementation of Stetson's DAOPHOTII algorithms and improvements to the sky fitting algorithms is briefly discussed and results obtained with the new algorithms for NOAO direct imaging data are shown. New interactive photometry catalog examining and editing tool PEXAMINE, and plans for future photometry catalog analysis tools...
Topics: NASA Technical Reports Server (NTRS), COMPUTER PROGRAMS, EDITING, IMAGING TECHNIQUES, STELLAR...
HSTphot, a photometry package designed to handle the undersampled PSFs found in WFPC2 images, is introduced and described, as well as some of the considerations that have to be made in order to obtain accurate PSF-fitting stellar photometry with WFPC2 data. Tests of HSTphot's internal reliability are made using multiple observations of the same field, and tests of external reliability are made by comparing with DoPHOT reductions of the same data. Subject headz'ngs: techniques: photometric
Topics: NASA Technical Reports Server (NTRS), DESIGN ANALYSIS, FABRICATION, STELLAR SPECTROPHOTOMETRY,...
Nine of the planetary nebulae observed by the Wisconsin filter photometers are compared with 15 Monocerotis in the spectral region 1430-4250 A. The data are corrected for the degradation of the filters of stellar photometer number four with time. Comparisons with simple models indicate that most of the observed nebulae are subject to some interstellar extinction in the far ultraviolet. However, NGC 246 and NGC 1360 appear to be nearly unreddened. Thus far no unexpected features have been found...
Topics: NASA Technical Reports Server (NTRS), OAO 2, PLANETARY NEBULAE, ULTRAVIOLET PHOTOMETRY,...
Data obtained from approximately 7500 ultraviolet television pictures are used to compile a celescope catalog of ultraviolet observations. This catalog lists the magnitude as observed in each of celescope's four ultraviolet color bands, the standard deviations of the observed ultraviolet magnitudes, positions, identifications, and ground based magnitudes, colors, and spectral types for approximately 5000 stars.
Topics: NASA Technical Reports Server (NTRS), ASTRONOMICAL CATALOGS, CELESCOPES, OAO 2, ULTRAVIOLET...
The machine-readable data file of The Absolute Calibration of Stellar Spectrophotometry as distributed by the Astronomical Data Center is described. The data file contains the absolute fluxes for 16 stars published in Tables 1 and 2 of Johnson (1980). The absolute calibrations were accomplished by combining the 13-color photometry calibrations of Johnson and Mitchell (1975) with spectra obtained with a Michelson spectrophotometer and covering the wavelength range 4000 to 10300 A (Johnson 1977)....
Topics: NASA Technical Reports Server (NTRS), ASTRONOMICAL CATALOGS, FLUX (RATE), STARS, STELLAR SPECTRA,...
Visual brightness measurements of SN 1987A are being obtained with the IUE acquisition camera and star tracker Fine Error Sensor, (FES) as part of each ultraviolet observation. Due to IUE's around-the-clock operation and lack of clouds, the FES record of SN 1987A provides the most complete set of visual photometry of the supernova made by any single instrument. The data illustrate the photometric limitations of the FES (+ or - 0.03 mag). Use of differential photometric methods are recommended...
Topics: NASA Technical Reports Server (NTRS), IUE, LIGHT CURVE, SPACEBORNE ASTRONOMY, STAR TRACKERS,...
The machine-readable version of the catalog, as it is currently being distributed from the astronomical data centers, is described. The catalog is a collection of spectrophotometric observations made using rotating grating scanners and calibrated with the fluxes of Vega. The observations cover various wavelength regions between about 330 and 1080 nm.
Topics: NASA Technical Reports Server (NTRS), ASTRONOMICAL CATALOGS, COMPUTER COMPATIBLE TAPES, STELLAR...
This is a compilation of abstracts of reports from Principal Investigators funded through NASA's Planetary Astronomy Program, Office of Space Science and Applications. The purpose is to provide a document which succinctly summarizes work conducted in this program for 1985. Each report contains a brief statement on the strategy of investigation and lists significant accomplishments within the area of the author's funded grant or contract, plans for future work, and publications.
Topics: NASA Technical Reports Server (NTRS), ASTEROIDS, COMETARY ATMOSPHERES, COMETS, INFRARED ASTRONOMY,...
At Lowell Observatory, precision photoelectric photometry was directed toward the study of solar variability and the variability of sun-like stars beginning in 1949 and continuing until now. The ubiquity and range of low-level variability, including some that appears to be cyclic, among solar-type stars shows that recent solar variability may be unusual only in its present restraint.
Topics: NASA Technical Reports Server (NTRS), G STARS, OBSERVATORIES, SOLAR ACTIVITY, STELLAR...
An extended series of photometric observations were made of the eclipsing variable CW Cephei using the Wisconsin instrument on OAO-2. Approximate elements which were derived based solely on the eclipse depths and shape of the secondary are in satisfactory agreement with those found using ground based observations. However, persistent asymmetries and anomalous light variations, all larger than the expected experimental error, were also found; subsequent ground-based observations show H sub alpha...
Topics: NASA Technical Reports Server (NTRS), CEPHEID VARIABLES, OAO 2, ULTRAVIOLET PHOTOMETRY, ECLIPSING...
Spectroscopic and photometric observations indicate a physical association between the peculiar early-type emission-line stars HD 122669 and HD 122691. The latter has undergone a drastic change in the strength of its emission lines during the past twenty years. There is some indication that both stars vary with shorter time scales.
Topics: NASA Technical Reports Server (NTRS), EARLY STARS, LINE SPECTRA, STELLAR SPECTROPHOTOMETRY,...
The four principal subgroups of the association were examined in detail using individual distances and reddening values determined for their B type members. Subgroup 1a appeared not to show a spread in age nor did it show a systematic distance increase with right ascension when fainter members were considered. An eastwardly increase in distance was found for subgroup 1b but the reddening law for the east Belt appeared normal. Small subclusterings in the vicinity of the Orion Nebula appeared not...
Topics: NASA Technical Reports Server (NTRS), ORION CONSTELLATION, STELLAR SPECTROPHOTOMETRY, B STARS,...
The magnetic tape version of the Catalog of Homogeneous Photometry of Bright Stars on the DDO System is described. The catalog represents a compilation of DDO photometry of 2196 bright G and K stars prepared from observations made at Kitt Peak National and Cerro Tololo Inter-American observatories. Stars representative of good velocities, spectral types, and freedom from companion contamination are presented.
Topics: NASA Technical Reports Server (NTRS), ASTRONOMICAL CATALOGS, COMPUTER COMPATIBLE TAPES, STELLAR...
Activities are presented for the grant-funded work at the Dominion Astrophysical (DAO) and Casleo Observatories. A comparison is planned for the spectrograms taken at both observatories of similar stars. It is reported that of the Northern Hemisphere program stars, only 112 Her remains to be analyzed. A preliminary solution for the components of this binary system has been found. The new ATLAS9 models have been used to reevaluate the effective temperatures and surface gravities derived for all...
Topics: NASA Technical Reports Server (NTRS), ASTRONOMICAL PHOTOGRAPHY, LINE SPECTRA, SPECTROGRAMS,...
High and low dispersion IUE data are analyzed in conjunction with coincident ground based spectrophotometric scans and supplementary infrared photometry of the symbiotic object AG Pegasi. The IUE observations yield an improved value of E(B-V) = 0.12. The two stellar components are easily recognized in the spectra. The cool component may be an M1.7 III star and the hot component appears to have T (sub eff) of approximately 30000 K. The emission lines observed in the ultraviolet indicate two or...
Topics: NASA Technical Reports Server (NTRS), RADIO ASTRONOMY, SPACEBORNE ASTRONOMY, STELLAR SPECTRA,...
A detailed description of the machine-readable version of the atlas as it is currently beng distributed from the Astronomical Data Center is given. The data were obtained with the Oke multichannel scanner on the 5-meter Hale reflector for purposes of synthesizing galaxy spectra, and the digitized atlas contains normalized spectral energy distributions, computed colors, scan line and continuum indices for 175 selected stars covering the complete ranges of spectral type and luminosity class. The...
Topics: NASA Technical Reports Server (NTRS), COLOR, SPECTRAL ENERGY DISTRIBUTION, STELLAR LUMINOSITY,...
The continued useful operation of the OAO-2 Wisconsin Experiment Package (WEP) for almost three years after its December 1968 launch is evidence of a superior engineering accomplishment. Reliability features of the experiment concept and design which have contributed to its long life are presented. Data anomalies and partial failures are summarized along with conclusions regarding their causes. The thermal, vacuum and radiation effects of the space environment are shown to be minimal and quite...
Topics: NASA Technical Reports Server (NTRS), ELECTRONIC PACKAGING, OAO 2, RELIABILITY ENGINEERING, STELLAR...
The appearance of the bright nova, Nova Serpentis 1970, provided the first opportunity to obtain spectrophotometric observations of a nova in the vacuum ultraviolet. OAO-2 carried out systematic measurements from shortly after outburst on through the first sixty days of nova activity. This data consist of filter photometry and spectral scans. General characteristics of the light and spectral variations in the ultraviolet exhibited by this set of data are described.
Topics: NASA Technical Reports Server (NTRS), NOVAE, OAO 2, SPECTRAL ENERGY DISTRIBUTION, ULTRAVIOLET...
The machine-readable version of the Atlas as it is currently being distributed from the Astronomical Data Center is described. The data were obtained with the Oke multichannel scanner on the 5-meter Hale reflector for purposes of synthesizing galaxy spectra, and the digitized Atlas contains normalized spectral energy distributions, computed colors, scan line and continuum indices for 175 selected stars covering the complete ranges of spectral type and luminosity class. The documentation...
Topics: NASA Technical Reports Server (NTRS), ARTIFICIAL INTELLIGENCE, ASTRONOMICAL CATALOGS, STELLAR...
A many-filter photometric technique for determining redshifts and morphological types, by fitting spectral templates to spectral energy distributions, has good potential for application in surveys. Despite success in studies performed on simulated data, the results have not been fully reliable when applied to real, low signal-to-noise data. We are investigating techniques to improve the fitting process.
Topics: NASA Technical Reports Server (NTRS), QUASARS, STELLAR SPECTROPHOTOMETRY, CHARGE COUPLED DEVICES,...
Line profiles were first obtained at maximum velocity separation of the spectroscopic binary Spica (alpha Vir), and then high resolution spectrophotometric images of selected features in the 1.1 micron spectrum of Comet Kohoutek were obtained in order to gain insight into the structures and variations in early-type star atmospheres.
Topics: NASA Technical Reports Server (NTRS), LINE SPECTRA, LYMAN ALPHA RADIATION, STELLAR ATMOSPHERES,...
The latest release of the IRAF (Image Reduction and Analysis Facility) MXTOOLS package includes the new tasks QDWFPC2 (Quick and Dirty Wide Field and Planetary Camera, which does quick CCD (charge-coupled device) stellar photometry on two Hubble Space Telescope (HST) WFPC2 (Wide Field and Planetary Camera) observations: WFPC2COLOR, which converts HST WFPC2 instrumental magnitudes to standard colors using the Holtzman et al. color equations, and QDCMD (Quick and Dirty Color Magnitude Diagram),...
Topics: NASA Technical Reports Server (NTRS), STELLAR SPECTROPHOTOMETRY, COMPUTER PROGRAMS, CCD CAMERAS,...
The Active Cavity Radiometer Irradiance Monitor (ACRIM) total-irradiance data from the Solar Maximum Mission have given a first comprehensive view of solar variability in the stellar sense. Five types of solar variability have been identified thus far. These have small amplitudes, less than a few tenths of one percent, and are at levels generally not yet detectable on other stars. The possible stellar analogs are interesting physically, and in particular may help us to understand solar behavior...
Topics: NASA Technical Reports Server (NTRS), IRRADIANCE, LUMINOSITY, RADIOMETERS, SOLAR ACTIVITY, SOLAR...
With a velocity dispersion of 370 + or - 50 km/sec the globular cluster system of M87 is kinematically hotter than the stars in the giant elliptical itself. This is consistent with the clusters' shallower density distribution for isotropic orbits. The mean metallicity of the 27 clusters in the sample analyzed here is no more than a factor of 2 more metal rich than the cluster system of the Milky Way, but considerably more metal poowr than the integrated starlight in the field at a radius of 1'...
Topics: NASA Technical Reports Server (NTRS), GLOBULAR CLUSTERS, SPECTROSCOPIC TELESCOPES, STELLAR...
Observed positions, proper motions, estimated photographic magnitudes and colors, and references to identifications in other catalogs are included. Photoelectric data on the UBV system are included for many stars, but no attempt was made to find all existing photometry. The machine-readable catalog is described.
Topics: NASA Technical Reports Server (NTRS), STELLAR MAGNITUDE, STELLAR MOTIONS, STELLAR...
Filter photometry has been used to derive the interstellar reddening law from stars through the study of a single spectral type, B0. The deficiency in the far ultraviolet flux of a supergiant relative to a main sequence star is compared with the difference in the flux distribution due to a change of one spectral class. Individual interstellar reddening curves show the general feature reported by Stecher (1969) and by Bless and Savage (1970). There is a large amount of scatter in the far...
Topics: NASA Technical Reports Server (NTRS), FLUX DENSITY, OAO 2, SUPERGIANT STARS, ULTRAVIOLET...
The surface brightness of the night sky has been measured at 12 wavelengths in the 1250-4300 A spectral region with the stellar photometers on OAO-2. From observations at high galactic latitudes it is possible to set upper limits on the brightness of the extragalactic sky background at several wavelengths. In the wavelength range 1420-1680 A the extragalactic background is not greater than 1.2 x 10 to the minus eight power cm/2 s/1 ster/1 A/1. Observations of near-by galaxies with OAO-2 are...
Topics: NASA Technical Reports Server (NTRS), EXTRATERRESTRIAL RADIATION, NIGHT SKY, OAO 2, SKY BRIGHTNESS,...
The ways in which the IUE has proved useful in studying highly evolved stars are reviewed. The importance of high dispersion spectra for abundance analyses of the sd0 stars and for studies of the wind from the central star of NGC 6543 and the wind from the 0 type component of Vela X-1 is shown. Low dispersion spectra are used for absolute spectrophotometry of the dwarf nova, Ex Hya. Angular resolution is important for detecting and locating UV sources in globular clusters.
Topics: NASA Technical Reports Server (NTRS), BINARY STARS, GLOBULAR CLUSTERS, IUE, STELLAR EVOLUTION,...
Observations were made with the International Ultraviolet Explorer of two quite diverse astronomical objects. The first is an extremely ultraviolet excess star projected near the globular cluster M5. The second is a previously unrecognized but very bright starburst galaxy. Each of these objects is discussed in detail.
Topics: NASA Technical Reports Server (NTRS), IUE, STAR CLUSTERS, STAR FORMATION, STELLAR SPECTRA,...
The ring-like interstellar visual echoes of radii 33 and 54 arcsec detected around SN 1987A should coincide with infrared echoes (thermal reradiation) from dust at T approximately equal to 15 to 30 K. Whether these infrared echoes are detectable at present is considered. They will be brightest at approximately 100 microns, the range of the Texas infrared photometer. Detectability depends on the ratio zeta congruent to tan(sub a)/tan(sub s)P(theta), where tan(sub a) and tan(sub s) are the visual...
Topics: NASA Technical Reports Server (NTRS), COSMIC DUST, INFRARED PHOTOMETRY, INFRARED REFLECTION, LIGHT...
The essential features of the calibration procedure can be divided into three parts. First, the shape of the bandpass of each photometer was determined by measuring the transmissions of the individual optical components and also by measuring the response of the photometer as a whole. Secondly, each photometer was placed in the essentially-collimated synchrotron radiation bundle maintained at a constant intensity level, and the output signal was determined from about 100 points on the objective....
Topics: NASA Technical Reports Server (NTRS), CALIBRATING, OAO 2, ULTRAVIOLET FILTERS, ULTRAVIOLET...
Spectrophotometric observations of emission line intensities were made in 8 positions in the planetary nebula NGC 7009. For the 6 brightest positions, the coverage is from 1400 A to 10,000 A. Standard equations used to correct for the existence of elements in other than the optical observable ionization stages give results over a wide range of ionization that are consistent and agree with abundances calculated using ultraviolet lines. This result is particularly gratifying for N because...
Topics: NASA Technical Reports Server (NTRS), ABUNDANCE, EMISSION SPECTRA, IONIZATION, LINE SPECTRA,...
Scans of lambda Lep, eta UMa, xi Dra, epsilon Dor, alpha Leo, phi Dra, upsilon Dra, beta Aur, alpha Pic and alpha Dor have been obtained with scanner OAO-2 over the range 1800-3600 A. These scans have been reduced to tracings of F sub lambda in the 20 A pass band vs. wavelength using a wavelength conversion scale and a relative spectral sensitivity function. The general trend of the relative flux plots compares well with the continua predicted by simple model atmospheres.
Topics: NASA Technical Reports Server (NTRS), A STARS, B STARS, OAO 2, STELLAR SPECTROPHOTOMETRY,...
We review the on-orbit spectroscopic observations that are being used to characterize the Charge Transfer Efficiency (CTE) of the STIS CCD in spectroscopic mode. We parameterize the CTE-related loss for spectrophotometry of point sources in terms of dependencies on the brightness of the source, the background level, the signal in the PSF outside the standard extraction box, and the time of observation. Primary constraints on our correction algorithm are provided by measurements of the CTE loss...
Topics: NASA Technical Reports Server (NTRS), CHARGE COUPLED DEVICES, STELLAR SPECTROPHOTOMETRY, CHARGE...
The user's guide is intended to enable astronomers to reduce the filter photometry data obtained by the WEP carried on the OAO 2 spacecraft. Only information related to the stellar photometer contained within the experiment package is presented, since the nebular photometer failed after 2-1/2 months of operation, while the stellar photometers provided roughly 49 months worth of data.
Topics: NASA Technical Reports Server (NTRS), INSTRUMENT PACKAGES, OAO 2, STELLAR SPECTROPHOTOMETRY, USER...
Diffuse galactic light has been observed with the four stellar photometers of the OAO-2 in 29 of Kapteyn's selected areas. The data can be understood in terms of a wavelength dependent albedo of the interstellar grains with a pronounced minimum around 2200 A with a rapid increase towards unity at wavelengths below 2000 A.
Topics: NASA Technical Reports Server (NTRS), GALACTIC RADIATION, INTERSTELLAR EXTINCTION, LIGHT...
An optical electronic facility is being used for meteor observations along with meteor radars and astronomical TV. The main parts of the facility are cameras using UM-92 optical electronic image tubes. The three cascade optical electronic image tube with magnetic focusing has a 40 mm cathode and resolution in the center of up to 30 pairs of lines/mm. The photocathode is of a multislit S-20 type. For meteor spectra observations, replica gratings of 200 and 300 lines/mm are used as the dispersive...
Topics: NASA Technical Reports Server (NTRS), METEOROID SHOWERS, OPTICAL EQUIPMENT, RADAR TRACKING,...
Stellar fluxes for 531 stars in the wavelength range lambda 5500-1330A lambda are presented in the form of graphs. The stars are divided into 52 different categories on the basis of their spectral types and objects within one category are shown together. The agreement between the various ultraviolet photometric systems for early type stars is generally better than 0.10 mag. Stars with known and/or observed variability have been grouped separately. A list of stars with observed photometric...
Topics: NASA Technical Reports Server (NTRS), ASTRONOMICAL CATALOGS, STARS, STELLAR SPECTRA, CHARTS,...
The C III 1909 A emission line in gamma 2 Velorum was observed over a period of 24 hours in an attempt to find short period time variability. Analysis of this data found no periods in the range of 0.5 to 200 minutes, and placed an upper limit of 3% on the amplitude of the stellar pulsations. Improved spectral resolution data for this line was obtained by offsetting the OAO-2 pointing in steps of 15 seconds of arc. The line profile derived by combining this offset data with the slit function...
Topics: NASA Technical Reports Server (NTRS), BINARY STARS, CARBON, LINE SPECTRA, OAO 2, STELLAR...
The largest body of data on ultraviolet spectra of late-type stars now available is the series of scans made with the long wavelength spectrometer onboard OAO-2. Some features of selected scans from this series and estimates of Mg II emission fluxes were reported earlier. Since that time, the effects of sky background, scattered light and variable instrumental sensitivity have become better understood. Additional stars are used to define more clearly the transition from Mg II 2800 A absorption...
Topics: NASA Technical Reports Server (NTRS), GIANT STARS, MAGNESIUM, OAO 2, SPECTRAL LINE WIDTH,...
