XMM-Newton RGS observation of V2491 Cyg

Details XMM-Newton RGS observation of V2491 Cyg XMM-Newton RGS observation of V2491 Cyg

Jun 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008atel.1561....1n&link_type=abstract

The Astronomer's Telegram, #1561

Astronomy and Astrophysics

Astronomy

9

X-Ray, Binaries, Cataclysmic Variables, Novae, Transients

Scientific paper

On 2008, May 20.6 (39.9 days after outburst) we obtained an XMM- Newton observation of the recent nova V2491 Cyg during the supersoft source (SSS) phase (Osborne et al. 2008, ATel #1542). The exposure time in the Reflection Grating Spectrometers (RGS) was 39.2ksec, and the average count rate in the RGS1 is 13.1 counts per sec (c/s). The light curve extracted from the RGS1 is highly variable.

Affiliated with

Also associated with

No associations

Rating

XMM-Newton RGS observation of V2491 Cyg 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 XMM-Newton RGS observation of V2491 Cyg, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and XMM-Newton RGS observation of V2491 Cyg will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1244498