Detection of radio emission at mas scales from HESS J0632+057 with the e-EVN

Details Detection of radio emission at mas scales from HESS J0632+057 with the e-EVN Detection of radio emission at mas scales from HESS J0632+057 with the e-EVN

Feb 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011atel.3180....1m&link_type=abstract

The Astronomer's Telegram, #3180

Astronomy and Astrophysics

Astronomy

7

Radio, X-Ray, >Gev, Tev, Vhe, Binary, Transient, Variables

Scientific paper

HESS J0632+057 is a variable TeV gamma-ray source (Aharonian et al. 2007, A&A, 469, L1, Acciari et al. 2009, ApJ, 698, L94). The likely low energy counterparts of the source are XMMU J063259.3+054801, the B0pe-type star MWC 148 (Hinton et al. 2009, ApJ, 690, L101), and a point-like probable non-thermal radio source (#3 in Skilton et al. 2009, MNRAS, 399, 317).
Falcone et al. 2011 (ATEL #3152) reported increased X-ray activity detected by Swift-XRT between January 23 and February 6, 2011 (MJD 55584-55598).

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