Swift XRT Observations of Circinus X-1

Details Swift XRT Observations of Circinus X-1 Swift XRT Observations of Circinus X-1

Aug 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008atel.1656....1p&link_type=abstract

The Astronomer's Telegram, #1656

Astronomy and Astrophysics

Astronomy

X-Ray, Binaries, Neutron Stars

Scientific paper

We report on a series of observations of the neutron star X-ray binary Circinus X-1, taken by Swift between 2 Jan 2004 until 1 August 2007. The observations were fit with single-component power-law and blackbody models. In both sets of fits, the column density of (partly interstellar) low- energy absorption was allowed to vary because Circinus X-1 is known to have a variable wind. The distance was assumed to be 8 kpc (Lei et al.

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