Chandra Grating Spectroscopy of Dwarf Novae

Details Chandra Grating Spectroscopy of Dwarf Novae Chandra Grating Spectroscopy of Dwarf Novae

Sep 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001cxo..prop..797w&link_type=abstract

Chandra Proposal ID #03300829

Physics

Chandra Proposal Id #03300829

Scientific paper

Dwarf novae are spectacular examples of accreting systems that have formed the basis of much of our understanding of accretion disks, from AGN to YSOs. Chandra grating observations have the power to resolve the temperature structure of the X-ray bright boundary layer for the first time, both in the optically-thin quiescent state and optically-thick outburst state, however only two systems have been observed to date. Here we propose to observe SU~UMa and VW~Hyi, the 2nd and 3rd brightest dwarf novae.

Affiliated with

Also associated with

No associations

Rating

Chandra Grating Spectroscopy of Dwarf Novae 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 Chandra Grating Spectroscopy of Dwarf Novae, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Chandra Grating Spectroscopy of Dwarf Novae will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1488211