The HMXRB system BD+37° 1160/4U 0515+38

Details The HMXRB system BD+37° 1160/4U 0515+38 The HMXRB system BD+37° 1160/4U 0515+38

Jan 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001adspr..28..395p&link_type=abstract

Advances in Space Research, Volume 28, Issue 2-3, p. 395-398.

Computer Science

Scientific paper

We present new optical data on BD+37° 1160, the optical counterpart of the X-ray source 1H0521+373 (=4U0515+38). The analysis of the stellar spectrum confirms that it is a very high mass object that probably experienced in the past several shell emission episodes. From the present optical data we find clear evidence of a new shell being ejected by the star. The hard spectrum of the X-ray source points to the presence of a compact companion. The similarity of the optical spectrum of BD+37° 1160 in the X-ray active phase with that of X Per strongly suggests that BD+37° 1160 is a BeXRB with a collapsed companion on a very wide orbit.

Affiliated with

Also associated with

No associations

Rating

The HMXRB system BD+37° 1160/4U 0515+38 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The HMXRB system BD+37° 1160/4U 0515+38, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The HMXRB system BD+37° 1160/4U 0515+38 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-921506