Evidence for a Black-Hole in Large Magellanic CLOUD-X-3

Details Evidence for a Black-Hole in Large Magellanic CLOUD-X-3 Evidence for a Black-Hole in Large Magellanic CLOUD-X-3

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984iaus..108..241c&link_type=abstract

Structure and Evolution of the Magellanic Clouds, Proceedings of IAU Symposium No. 108, held 5-8 September 1983 in Tübingen, Wes

Computer Science

Scientific paper

Spectroscopy of the optical counterpart of LMC X-3 reveals a slightly
reddened B3 V star. An orbital analysis shows that the unseen companion
star must have a mass larger than the B star and should easily be
detected in the spectrum, if it were a normal star. Thus it appears that
this object is a very good candidate for a black hole.

Affiliated with

Also associated with

No associations

Rating

Evidence for a Black-Hole in Large Magellanic CLOUD-X-3 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 Evidence for a Black-Hole in Large Magellanic CLOUD-X-3, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Evidence for a Black-Hole in Large Magellanic CLOUD-X-3 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1395241