C H A N D R A
S C I E N C E
C E N T E R O B S E R V A T I O N C A T A L O G |
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Abstract: 4U 1543-475 is a recurrent black hole X-ray binary. It is one of the few sources with a dynamically confirmed mass, and measured distance (M = 9.4 +/- 2.0 Msun, distance = 7.5 +/- 1.0 kpc; Park et al. 2004). This means that it is a rare case wherein black hole spin can be measured using continuum fitting. The source has risen very quickly from the detection of renewed activity only (up to 2.5-3 Crab in just 2-3 days, see ATEL 14701). It is now in the soft state, which is the one wherein spin can be measured as other contributions to the continuum are minimal. In this state, disk winds and UFOs can also be detected using the HETGS. With the ACIS-S array in CC mode, Chandra is uniquely able to observe a source this bright without distortions. |
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