Swift does not detect a source near H 1743-322

Details Swift does not detect a source near H 1743-322 Swift does not detect a source near H 1743-322

Apr 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011atel.3295....1m&link_type=abstract

The Astronomer's Telegram, #3295

Astronomy and Astrophysics

Astronomy

Binary, Black Hole, Transient

Scientific paper

A low-frequency oscillation with a period of approximately 91 s was visible in the RXTE/PCA light curve of the black-hole candidate H1743-322 (ATel #3277), in outburst since April 6, 2011 (ATel #32763) and currently in hard state. The oscillation was detected only in the first RXTE observation (performed 16:05:01 (UTC) on April 12, 2011). The hypothesis that the oscillations are due to a second active source in the PCA field of view was put forward.

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