Optical Spectroscopy of the transient pulsar and Be/X-ray binary V0332+53

Details Optical Spectroscopy of the transient pulsar and Be/X-ray binary V0332+53 Optical Spectroscopy of the transient pulsar and Be/X-ray binary V0332+53

Oct 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008atel.1803....1h&link_type=abstract

The Astronomer's Telegram, #1803

Astronomy and Astrophysics

Astronomy

3

Optical, Binaries, Cataclysmic Variables, Pulsars, Transients, Variables

Scientific paper

We report on post X-ray outburst (ATEL #1792) observations of the transient pulsar and Be/X-ray binary V0332+53 (BQ Cam). We obtained an optical spectrum (range 4700-7000 Angstroms, resolution 3 Angstroms) on October 22.54 UT using the 1.82-m Plaskett Telescope of the National Research Council of Canada. The spectrum shows a strong (FWHM 12 Angstroms) H-alpha emission with P-Cygni profile. The blue absorption component is shifted ~1600 km/s.

Affiliated with

Also associated with

No associations

Rating

Optical Spectroscopy of the transient pulsar and Be/X-ray binary V0332+53 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 Optical Spectroscopy of the transient pulsar and Be/X-ray binary V0332+53, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Optical Spectroscopy of the transient pulsar and Be/X-ray binary V0332+53 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-774616