Chandra and XMM-Newton Observations of the Gamma-ray Binary 1FGL J1018.6-5856

Details Chandra and XMM-Newton Observations of the Gamma-ray Binary 1FGL J1018.6-5856 Chandra and XMM-Newton Observations of the Gamma-ray Binary 1FGL J1018.6-5856

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011atel.3228....1p&link_type=abstract

The Astronomer's Telegram, #3228

Astronomy and Astrophysics

Astronomy

8

Optical, X-Ray, Gamma Ray, >Gev, Binary, Neutron Star

Scientific paper

The Fermi LAT source 1FGL J1018.6-5856 has been recently identified as a high-mass gamma-ray binary (Corbet et al., ATel #3221). The source was observed with Chandra ACIS-I (ObsID 11831) on 2010-08-17 from 01:17 to 04:04 UTC, which corresponds to the binary phase interval from 0.312 to 0.319 (phase uncertainty ±0.024; zero phase corresponds to the gamma-ray flux maximum at the reference epoch MJD 55403.3+/-0.4, period 16.58+/-0.04 d, according to ATel #3221).

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