A state change of H1743-322 confirmed by INTEGRAL observations

Details A state change of H1743-322 confirmed by INTEGRAL observations A state change of H1743-322 confirmed by INTEGRAL observations

Oct 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008atel.1808....1p&link_type=abstract

The Astronomer's Telegram, #1808

Astronomy and Astrophysics

Astronomy

2

X-Ray, Gamma Ray, Binaries, Black Holes, Neutron Stars, Transients

Scientific paper

The last INTEGRAL observations from the Galactic Center (GC) and Galactic Bulge (GB) programs confirm the state transition undergone by H1743-322 into a softer state (Atel #1804). Since its renewed activity spotted on UT 2008 Sep 23 (See Atel #1739), H1743-322 was followed every ~2 days by INTEGRAL as part of these two programs (Atel #1745), and as part of ToO observations (Atel #1779, #1798).

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