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Four-colour and H-beta photometry of blue stars selected from a balloon-ultraviolet survey and other sources
New uvby and/or H-beta photometry is obtained at the Chiranhigh-altitude outstation for 105 stars. Certain of the program stars areselected from a comparison of the SCAP 2000 balloon-ultraviolet skysurvey of the Laboratoire d'Astronomie Spatiale with the correspondingblue and red prints of the Palomar Observatory sky survey. Only a smallportion of these stars turn out to be B stars, whereas, the rest of thestars, which are selected from a variety of other sources, are mostly Bstars and if of normal luminosity are in many cases many Population Iscale heights from the galactic plane. It is shown that theidentification of B stars is practicable only at a good observing siteand that if H-beta photometry is also obtained, sdOB, sdB, and hothorizontal branch B stars can be distinguished from normal stars bytheir position in the beta/c(0) diagram.
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Membre dels grups següents:
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Dades d'Observació i Astrometria
| Constel·lació: | Aries |
| Ascensió Recta: | 02h09m50.91s |
| Declinació: | +26°29'04.3" |
| Magnitud Aparent: | 8.524 |
| Distancia: | 228.833 parsecs |
| Moviment propi RA: | 20 |
| Moviment propi Dec: | -10.2 |
| B-T magnitude: | 9.083 |
| V-T magnitude: | 8.571 |
Catàlegs i designacions:
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