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Massive eclipsing binary candidates
New UBV data are provided for 63 southern OB stars which are eitheridentified in the survey by Garrison, Hiltner, and Schild as havingdouble lines or are known from Wood et al. to be eclipsing binaries.Twenty of the stars are known eclipsing variables. Four stars, notpreviously known as eclipsing, have both spectroscopic evidence ofduplicity and significant photometric variations. Several additionalstars have a marginally significant spread in V magnitude.
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Membre dels grups següents:
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Dades d'Observació i Astrometria
| Constel·lació: | Ara |
| Ascensió Recta: | 17h48m17.28s |
| Declinació: | -47°15'18.4" |
| Magnitud Aparent: | 7.115 |
| Distancia: | 137.741 parsecs |
| Moviment propi RA: | 1.3 |
| Moviment propi Dec: | 6.6 |
| B-T magnitude: | 7.306 |
| V-T magnitude: | 7.131 |
Catàlegs i designacions:
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