Increased X-ray activity and likely binary period of HESS J0632+057 Observed by Swift-XRT

Details Increased X-ray activity and likely binary period of HESS J0632+057 Observed by Swift-XRT Increased X-ray activity and likely binary period of HESS J0632+057 Observed by Swift-XRT

Feb 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011atel.3152....1f&link_type=abstract

The Astronomer's Telegram, #3152

Astronomy and Astrophysics

Astronomy

7

Optical, X-Ray, >Gev, Tev, Vhe, Binary

Scientific paper

HESS J0632+057 (R.A. 06:32:58.3, Dec. +05:48:20), which is associated
with XMMU J063259.3+054801 and Be star MWC 148 (R.A. 06:32:59.3, Dec.
+05:48:01) has shown a recent increase in X-ray activity, based on
Swift-XRT monitoring data.

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