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Ultraviolet and optical studies of binaries with luminous cool primaries and hot companions. IV - Further IUE detections
We have obtained IUE spectra for 31 middle and late-type giant andsupergiant stars whose TD-1 fluxes or ground-based spectra indicate thepresence of a hot component, or whose radial velocities indicate anunseen component. Stellar components earlier than type F1 were detectedin 22 cases. While 20 of the hot secondaries are seen weakly in opticalspectra, two are UV discoveries: HD 58134 and HD 183864. The hotcompanions are classified accurately by temperature class from theirfar-UV spectra. The interstellar extinction of each system and therelative luminosities of the components are derived from the UV andoptical fluxes, using a new grid of UV intrinsic colors for hot dwarfs.We find that many giant stars apparently have companions which are toohot and hence too luminous for consistency with the primary's spectralclassification.
| Further IUE Detections of Hot Companions to Cool Stars
Many late-type giants and supergiants have companion stars still on theupper main sequence, but barely detectable in ground-based observations.In 1989-90 we continued our surveys of suspected hot companions with theIUE satellite. Of 32 spectrum binaries or SB1 systems observed, 25reveal clear signatures in the UV of a B or A type component. The far-UVspectra are easily classified by temperature class with respect to IUEstandard stars. Some of the more significant new results: ground UVspectrosc. HD no. V spectral type type binary? Note---------------------------------------------------------- 25555 5.47 G0III + A4 dB8+ var 32835/6 7.65 F5 V + A dB8.5 a 37269AB 5.40 G5 III: +A3 d:A0 var 49126 7.28 F8 IV-V + B9.5 dB8.5 a 52690 6.55 M1 Ib + A-BgB8- 58134 7.64: G5 Ib g:A1- p 63208 6.18 G2 III + A4 gB9.5 var? 1675168.46 G5 III + A -- b 183864 7.32 G2 Ib d:A0 296.0d 218600 8.39 F2 Ib + A-- b In two systems the ground-based luminosity classifications of theirprimaries are seriously inconsistent with their upper main sequencecompanions (note a). Two spectrum binaries with supposedly A-typesecondaries show no evidence of such in the UV (note b). Several othercases demonstrate a trend in our surveys: although some classificationsare confirmed, we frequently find that the IUE spectral class is hotterthan the ground estimate by 2 or more subclasses. This work is supportedunder NASA contract NAS 5-28749. SBP is a staff member of the SpaceTelescope Science Institute. TBA is a member of the GHRS Science Team.
| New UBVRI photometry for 900 supergiants
A description is presented of the results obtained in connection with asystematic program of supergiant photometry on the Johnson UBVRI system.During the eight years after the start of the program, almost 1000 starshave been observed, about 400 three or more times each. The originalselection of stars used the spectral type catalog of Jaschek et al.(1964) to choose supergiants. Since observations were possible from bothChile and Canada, no declination limits were imposed, and no particularselection criteria were imposed other than to eliminate carbon stars.These are so red as to require enormous extrapolations of thetransformation equations.
| Spectral Classification of Stars Noted on Case Objective-Prism Plates. I
Not Available
| Magnitudes and colors for 833 Northern and Southern stars.
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1955AJ.....60...65E&db_key=AST
| A Finding List of F Stars of High Luminosity.
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1952ApJ...115..475N&db_key=AST
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