The radio counterpart of the likely TeV binary HESS J0632+057

Skilton JL, Pandey-Pommier M, Hinton JA, Cheung CC, Aharonian FA, Brucker J, Dubus G, Fiasson A, Funk S, Gallant Y, Marcowith A, Reimer O (2009)


Publication Type: Journal article

Publication year: 2009

Journal

Book Volume: 399

Pages Range: 317-322

Journal Issue: 1

DOI: 10.1111/j.1365-2966.2009.15272.x

Abstract

The few known gamma-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 I 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, alpha, of similar to 0.6. In the VLA data there is significant flux variability oil similar to month time-scales around the mean flux density of approximate to 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 gamma-ray binary systems.

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APA:

Skilton, J.L., Pandey-Pommier, M., Hinton, J.A., Cheung, C.C., Aharonian, F.A., Brucker, J.,... Reimer, O. (2009). The radio counterpart of the likely TeV binary HESS J0632+057. Monthly Notices of the Royal Astronomical Society, 399(1), 317-322. https://doi.org/10.1111/j.1365-2966.2009.15272.x

MLA:

Skilton, J. L., et al. "The radio counterpart of the likely TeV binary HESS J0632+057." Monthly Notices of the Royal Astronomical Society 399.1 (2009): 317-322.

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