Volume 533, September 2011
|Number of page(s)||4|
|Published online||24 August 2011|
Letter to the Editor
Revealing the extended radio emission from the gamma-ray binary HESS J0632+057
Departament d’Astronomia i MeteorologiaInstitut de Ciències del Cosmos (ICC), Universitat de Barcelona (IEEC-UB), Martí i Franquès 1, 08028 Barcelona, Spain
e-mail: email@example.com; firstname.lastname@example.org; email@example.com
Received: 25 July 2011
Accepted: 12 August 2011
Context. After the detection of a 321-day periodicity in X-rays, HESS J0632+057 can be robustly considered a new member of the selected group of gamma-ray binaries. These sources are known to show extended radio structure on scales of milliarcseconds (mas).
Aims. We present the expected extended radio emission on mas scales from HESS J0632+057.
Methods. We observed HESS J0632+057 with the European VLBI Network (EVN) at 1.6 GHz in two epochs: during the January/February 2011 X-ray outburst and 30 days later.
Results. The VLBI image obtained during the outburst shows a compact ~0.4 mJy radio source, whereas 30 days later the source has faded and appears extended, with a projected size of ~75 AU. The peak of the emission is displaced between runs 21 ± 5 AU, which is bigger than the orbit size. The position of the radio source is compatible with the Be star MWC 148, which sets the proper motion of the binary system below 3 mas yr-1 in each coordinate. The brightness temperature of the source is above 2 × 106 K. We compare the multiwavelength properties of HESS J0632+057 with those of the previously known gamma-ray binaries.
Conclusions.HESS J0632+057 displays extended and variable non-thermal radio emission. Its morphology, size, and displacement on AU scales are similar to those found in the other gamma-ray binaries, PSR B1259 − 63, LS 5039, and LS I +61 303, supporting a similar nature for HESS J0632+057.
Key words: radio continuum: stars / X-rays: binaries / stars: emission-line, Be / gamma rays: stars / stars: individual: MWC148
© ESO, 2011
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