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Einstein Observatory magnitude-limited X-ray survey of late-type giant and supergiant stars
Results are presented of an extensive X-ray survey of 380 giant andsupergiant stars of spectral types from F to M, carried out with theEinstein Observatory. It was found that the observed F giants orsubgiants (slightly evolved stars with a mass M less than about 2 solarmasses) are X-ray emitters at the same level of main-sequence stars ofsimilar spectral type. The G giants show a range of emissions more than3 orders of magnitude wide; some single G giants exist with X-rayluminosities comparable to RS CVn systems, while some nearby large Ggiants have upper limits on the X-ray emission below typical solarvalues. The K giants have an observed X-ray emission level significantlylower than F and F giants. None of the 29 M giants were detected, exceptfor one spectroscopic binary.
| Photoelectric photometry of late type stars in the direction opposed to galactic rotation
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1974A&AS...16..269G&db_key=AST
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Observation and Astrometry data
| Constellation: | Vela |
| Right ascension: | 09h23m05.98s |
| Declination: | -53°49'12.6" |
| Apparent magnitude: | 6.817 |
| Distance: | 246.914 parsecs |
| Proper motion RA: | -8.8 |
| Proper motion Dec: | 7.5 |
| B-T magnitude: | 8.121 |
| V-T magnitude: | 6.925 |
Catalogs and designations:
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