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The results of observations of 159 stars at 1640 A in Puppis made withthe space telescope 'Glazar' are presented. It is shown that theobserved stars are members of different groups of stars situated atdistances of about 120, 370, 700, 1250, 2400, and 4000 pc. The last twogroups belong to the Pup OB1 and Pup OB2 stellar associations. There isrelatively little absorption in the observed region. The absorbingmatter is mainly concentrated in small clouds. It is suggested thatthree stars - CP - 27 deg 4197, HD 60479, and HD 61672 - are embedded ina dust envelope and that the star HD 60057 has a hot subdwarf companion.Forty-four of the observed stars are new OB or early A-type stars,spectral types of which were not known.
| Walraven photometry of nearby southern OB associations
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Miembro de los siguientes grupos:
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Datos observacionales y astrométricos
| Constelación: | Can Mayor |
| Ascensión Recta: | 07h17m48.33s |
| Declinación: | -28°17'10.5" |
| Magnitud Aparente: | 8.321 |
| Distancia: | 2941.176 parsecs |
| Movimiento Propio en Ascensión Recta: | -7.4 |
| Movimiento Propio en Declinación: | 8.5 |
| B-T magnitude: | 8.26 |
| V-T magnitude: | 8.316 |
Catálogos y designaciones:
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