XMM-Newton Proposal 03047202

Details XMM-Newton Proposal 03047202 XMM-Newton Proposal 03047202

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004xmm..prop..157o&link_type=abstract

XMM-Newton Proposal ID #03047202

Physics

White Dwarf Binaries, Neutron Star Binaries, Cataclysmic Variables, Ulxs, Black Holes, V4743 Sgr, Rx J0533.7-7034, Xmm-Newton Proposal 03047202

Scientific paper

We propose monitoring observations of supersoft X-ray sources. The classical nova V4743 Sgr, for which the best spectra of a luminous supersoft X-ray source have ever been obtained, should be monitored once again during the coming year, also in order to measure the length of hydrogen burning. We then propose that RX J0533.7-7034, a transient source observed for a few months in the LMC and never found to be luminous again, should be observed in five short snapshot exposures (every two and a half months) so that we may determine whether it underwent a hydrogen shell flash, and what its recurrence time scale may be.

Affiliated with

Also associated with

No associations

Rating

XMM-Newton Proposal 03047202 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 03047202, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and XMM-Newton Proposal 03047202 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1474301