Doppler tomography of the rise to outburst in IY UMa

Details Doppler tomography of the rise to outburst in IY UMa Doppler tomography of the rise to outburst in IY UMa

Jan 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aspc..261..537r&link_type=abstract

The Physics of Cataclysmic Variables and Related Objects, ASP Conference Proceedings, Vol. 261. Edited by B. T. Gänsicke, K. Beu

Physics

4

Scientific paper

Time-resolved spectroscopy of the SU UMa system IY UMa shortly before
and during the early stages of a normal outburst reveals dramatic
changes in the accretion flow. Through Doppler tomography we study the
emission distribution and conclude that reprocessing of boundary layer
radiation is the dominant emission line mechanism in outburst.

Affiliated with

Also associated with

No associations

Rating

Doppler tomography of the rise to outburst in IY UMa 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 Doppler tomography of the rise to outburst in IY UMa, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Doppler tomography of the rise to outburst in IY UMa will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1087714