A 6.8 Day Period in IGR J16493-4348 from Swift/BAT and RXTE/PCA Observations

Details A 6.8 Day Period in IGR J16493-4348 from Swift/BAT and RXTE/PCA Observations A 6.8 Day Period in IGR J16493-4348 from Swift/BAT and RXTE/PCA Observations

May 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atel.2599....1c&link_type=abstract

The Astronomer's Telegram, #2599

Astronomy and Astrophysics

Astronomy

X-Ray, Binaries, Black Holes, Neutron Stars, Variables, Stars

Scientific paper

IGR J16493-4348 was discovered by Grebenev et al. (2005, ATel #457) and
subsequent X-ray observations suggested that the source is an X-ray
binary (e.g. Hill et al. 2008, MNRAS, 385, 423).

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