(Received July 2, 1996)
An eclipsing binary system with an orbital period of 33
108, whose light varies over the range 16
8
17
8 in B has been detected among the high-luminosity blue stars in M 33. One of the components apparently exhibits intrinsic variability with a small amplitude. The star lies at the center of a bipolar nebula seen in H
. The system is assumed to contain an accretion disk. © 1997 MAIK/Interperiodika
| History | Received: July 2, 1996 |
| Subject | Stars |
| PACS |
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| Keywords | eclipsing binary stars; luminescence; accretion disks; galaxies; H II regions |
| Doc. Type | Experimental |
| Coden | ALETEO |