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Near-infrared photometry of stars
Results are presented of infrared photometric observations performed oncomparison stars during a monitoring of long-period variables. Theseobservations, spread over a lapse of about 5 years, are used to derivethe J, H, and K magnitudes of 54 stars in the photometric systemdescribed by Koornneef (1983). The 1950.0 coordinates, spectral types,visual magnitudes, average magnitudes, and the number of observationsare given for each object.
| 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.
| Photometric standard sequences in Carina iII = 275° - 295°
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| Takýmyýldýz: | Karina |
| Sað Açýklýk: | 10h28m48.01s |
| Yükselim: | -57°13'58.8" |
| Görünürdeki Parlaklýk: | 6.689 |
| Uzaklýk: | 160.256 parsek |
| özdevim Sað Açýklýk: | -17.1 |
| özdevim Yükselim: | 19.5 |
| B-T magnitude: | 8.026 |
| V-T magnitude: | 6.8 |
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