XMM-Newton Proposal 03016001

Details XMM-Newton Proposal 03016001 XMM-Newton Proposal 03016001

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004xmm..prop...54g&link_type=abstract

XMM-Newton Proposal ID #03016001

Physics

Stars, White Dwarfs, Solar System, V1647 Ori, Xmm-Newton Proposal 03016001

Scientific paper

Our CXO and XMM follow-ups of the outburst of V1647 Ori have shown strongly enhanced variable X-ray emission, occuring as a consequence of the high disk accretion rate. Our analysis of the combined X-ray datasets indicates that X-rays emerge with a 0.7 day periodicity, which is consistent with a modulation by the Keplerian rotation of the inner accretion disk. New longer X-ray observations are crucial to confirm this periodicity because, if correct, this result provides a unique view of the source of high energy emission and would dramatically confirm that the X-ray outburst of V1647 Ori emerges from the star-disk interaction region. Moreover, the new X-ray absorption measurement will allow a temporal study of the mass-loss. We request a 120 ks XMM/EPIC exposure on V1647 Ori on 2005 April 5.

Affiliated with

Also associated with

No associations

Rating

XMM-Newton Proposal 03016001 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 Proposal 03016001, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and XMM-Newton Proposal 03016001 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1474023