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Bright blue stars in VELA observed with the 'Glazar' space telescope
Seventy-one stars brighter than about 9 m have been detected at 1640 Ain the Vela region with the space telescope Glazar. It is shown thatmost of the detected stars belong to a B-type stellar association at adistance of 460 pc and to two OB stellar associations at distances of1100 pc and 1700 pc. The existence of B-type stellar association at adistance of 110 pc is suspected. A new O-type star cluster, which is apossible nucleus of the OB stellar association at 1700 pc, has beendetected. The distribution of the absorbing matter in the observed areais studied. We presume that the stars HD 75 063 and 76 534 are probablyembedded in a circumstellar dust shell. All observed stars, includingthose with unknown spectra, are early type stars.
| Hα-EMISSION Stars and Planetary Nebulae in the Vicinity of m8 and M20 and in VELA from L = 230° to 241° Along the Galactic Equator.
Abstract image available at:http://adsabs.harvard.edu/abs/1957ApJ...126..302V
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Observation and Astrometry data
| Constellation: | Segel des Schiffs |
| Right ascension: | 08h51m26.03s |
| Declination: | -45°37'22.6" |
| Apparent magnitude: | 7.747 |
| Distance: | 209.205 parsecs |
| Proper motion RA: | -10.1 |
| Proper motion Dec: | 13.7 |
| B-T magnitude: | 7.751 |
| V-T magnitude: | 7.748 |
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