Measuring the disk wind in the Galactic superluminal source GRO J1655-40

Details Measuring the disk wind in the Galactic superluminal source GRO J1655-40 Measuring the disk wind in the Galactic superluminal source GRO J1655-40

Oct 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005xmm..prop..218s&link_type=abstract

XMM-Newton Proposal ID #04058501

Physics

White Dwarf Binaries, Neutron Star Binaries, Cataclysmic Variables, Ulxs, Black Holes, Gro J1655-40, Xmm-Newton Proposal 04058501

Scientific paper

The Galactic superluminal source GRO J1655-40 is a binary system containing a 7 M_sun black hole. XMM-Newton observations during high/soft state in March 2005 have shown clear He-like Fe absorption lines in the EPIC spectra, while RGS has provided the first high resolution spectra of the source, showing absorption features at 0.7 keV, probably due to blueshifted Fe XVIII. We propose triggered observations of GRO J1655-40 both in a new high state, as well as in the very high and low states, aimed to follow the evolution of these absorption features, study their dependence with the X-ray intensity and determine the nature of the absorber.

Affiliated with

Also associated with

No associations

Rating

Measuring the disk wind in the Galactic superluminal source GRO J1655-40 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 Measuring the disk wind in the Galactic superluminal source GRO J1655-40, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Measuring the disk wind in the Galactic superluminal source GRO J1655-40 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1660064