Physics – Nuclear Physics
Scientific paper
Jun 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004nuphs.132..668y&link_type=abstract
Nuclear Physics B Proceedings Supplements, Volume 132, p. 668-671.
Physics
Nuclear Physics
1
Scientific paper
The RXTE public observations of the outbursts of black hole soft X-ray transients XTE J1550-564, XTE J1859+226, 4U 1630-47, XTE J1118+480, XTE J1650-500, and the neutron star soft X-ray transients 4U 1608-52, Aquila X-1, including a variable `persistent' neutron star low mass X-ray binary 4U 1705-44, are summarized in this paper. The hard X-ray view of those outbursts, which is quite different from that of the soft X-ray band, suggests that there are several types of outbursts which result in different hard X-ray outburst profile - the outburst profiles are energy dependent. One type is the low/hard state outbursts, the other type is the outburst showing transitions from the low/hard state to the high/soft state, or to the intermediate or to the very high state. The later has an initial low/hard state, introducing the phenomena that the hard X-ray precedes the soft X-ray in the outburst rise. Such outbursts in XTE J1550-564, Aql X-1 and 4U 1705-44 support a two-accretion-flow model which involves one Keplerian disk flow and one sub-Keplerian flow for the initial outburst rise.
No associations
LandOfFree
Black hole and neutron star soft X-ray transients: a hard X-ray view of their outbursts 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 Black hole and neutron star soft X-ray transients: a hard X-ray view of their outbursts, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Black hole and neutron star soft X-ray transients: a hard X-ray view of their outbursts will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1392747