Be Star Counterpart of X-ray Transient IGR J01583+6713

Astronomy and Astrophysics – Astronomy

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

3

Optical, X-Ray, Binaries, Transients

Scientific paper

Kennea et al. (ATel #673) proposed an optical/IR candidate for the hard X-ray transient IGR J01583+6713 (Steiner et al., ATel #672) based on its positional coincidence with a Swift XRT source detection. The USNO-B1.0 POSS II magnitudes of the star are B=14.98, R=13.24, I=12.12. It is located at RA = 01h 58m 18.44s, Decl. = +67d 13' 23.5" (J2000). We obtained a low-resolution optical spectrum using the MDM 2.4m telescope on 2005 Dec.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Be Star Counterpart of X-ray Transient IGR J01583+6713 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 Be Star Counterpart of X-ray Transient IGR J01583+6713, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Be Star Counterpart of X-ray Transient IGR J01583+6713 will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1035656

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.