Please use this identifier to cite or link to this item: http://hdl.handle.net/2381/21001
Title: The radio counterpart of the likely TeV binary HESS J0632+057
Authors: Skilton, J. L.
Hinton, J. A.
Pandey-Pommier, M.
Cheung, C. C.
Aharonian, F. A.
Brucker, J.
Dubus, G.
Fiasson, A.
Gallant, Y.
Marcowith, A.
Fiasson, A.
Funk, S.
Reimer, O.
First Published: 11-Oct-2009
Publisher: Oxford University Press (OUP)
Citation: Monthly Notices of the Royal Astronomical Society, 2009, 399 (1), pp. 317-322
Abstract: The few known γ-ray binary systems are all associated with variable radio and X-ray emission. The TeV source HESS J0632+057, apparently associated with the Be star MWC 148, is plausibly a new member of this class. Following the identification of a variable X-ray counterpart to the TeV source we conducted Giant Metrewave Radio Telescope (GMRT) and Very Large Array (VLA) observations in 2008 June–September to search for the radio counterpart of this object. A point-like radio source at the position of the star is detected in both 1280-MHz GMRT and 5-GHz VLA observations, with an average spectral index, α, of ∼0.6. In the VLA data there is significant flux variability on ∼month time-scales around the mean flux density of ≈0.3 mJy. These radio properties (and the overall spectral energy distribution) are consistent with an interpretation of HESS J0632+057 as a lower power analogue of the established γ-ray binary systems.
DOI Link: 10.1111/j.1365-2966.2009.15272.x
ISSN: 0035-8711
eISSN: 1365-2966
Links: http://hdl.handle.net/2381/21001
http://mnras.oxfordjournals.org/content/399/1/317
Version: Publisher Version
Status: Peer-reviewed
Type: Journal Article
Rights: This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2009 the authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved. Deposited with reference to the publisher’s archiving policy available on the SHERPA/RoMEO website.
Appears in Collections:Published Articles, Dept. of Physics and Astronomy

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