XMM-Newton Proposal 03040101

Details XMM-Newton Proposal 03040101 XMM-Newton Proposal 03040101

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004xmm..prop..142o&link_type=abstract

XMM-Newton Proposal ID #03040101

Computer Science

White Dwarf Binaries, Neutron Star Binaries, Cataclysmic Variables, Ulxs, Black Holes, Cp Pup, Xmm-Newton Proposal 03040101

Scientific paper

We propose to observe the quiescent nova CP Pup and the peculiar dwarf nova EY Cyg, that shows signatures of a past nova explosion. These two systems are known X-ray sources at low inclination, so they are ideal targets to study how accretion occurs. CP Pup has a short orbital period, while EY Cyg is a long period systems, allowing a useful comparison. Spectroscopy will be used to measure mdot and test theories of secular evolution, timing analysis will be used to localize and constrain the size of the emitting region.

Affiliated with

Also associated with

No associations

Rating

XMM-Newton Proposal 03040101 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 03040101, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and XMM-Newton Proposal 03040101 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1474269