XMM-Newton Observations of Black Hole X-ray Transients in Quiescence

Details XMM-Newton Observations of Black Hole X-ray Transients in Quiescence XMM-Newton Observations of Black Hole X-ray Transients in Quiescence

Feb 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005tmgm.meet.1273h&link_type=abstract

The Tenth Marcel Grossmann Meeting. Proceedings of the MG10 Meeting held at Brazilian Center for Research in Physics (CBPF), Rio

Physics

Scientific paper

X-ray observations of black hole X-ray transients in their quiescent
phase show that transient systems containing neutron stars are
significantly dimmer than those containing black holes, as expected
since black holes have no solid surface, in agreement with the
predictions of the Advection Dominated Accretion Flow (ADAF) models.

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