Probable Optical Counterpart of IGR J00234+6141

Details Probable Optical Counterpart of IGR J00234+6141 Probable Optical Counterpart of IGR J00234+6141

Jan 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006atel..709....1h&link_type=abstract

The Astronomer's Telegram, #709

Astronomy and Astrophysics

Astronomy

7

Optical, X-Ray, Cataclysmic Variables

Scientific paper

We report a probable identification of the weak hard X-ray source IGR J00234+6141 (den Hartog et al., ATel #394) with a star that has an optical spectrum of a cataclysmic variable. den Hartog et al. noted the presence of a ROSAT All-Sky Survey source 1RXS J002258.3+614111 located 3.15' from the INTEGRAL position and marginally consistent with it, given the estimated 3' error radius (90% confidence) of the latter.

Affiliated with

Also associated with

No associations

Rating

Probable Optical Counterpart of IGR J00234+6141 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 Probable Optical Counterpart of IGR J00234+6141, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Probable Optical Counterpart of IGR J00234+6141 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1202301