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dc.contributorDepartment of Physics & Astronomy, University College London, Gower Street, London, WC1E 6BT, UK
dc.contributorDepartment of Physics & Astronomy, University College London, Gower Street, London, WC1E 6BT, UK; Astrophysics Group, Cavendish Laboratory, University of Cambridge, Cambridge, UK
dc.contributorRoyal Observatory of Belgium, Ringlaan 3, 1180, Brussels, Belgium
dc.contributorHarvard-Smithsonian Centre for Astrophysics, 60 Garden Street, Cambridge, MA, 02138, USA
dc.contributorJeremiah Horrocks Institute, University of Central Lancashire, Preston, PR1 2HE, UK; Faculty of Computing, Engineering and Science, University of South Wales, Pontypridd, CF37 1DL, UK
dc.contributorUK ARC Node, JBCA, Alan Turing Building, University of Manchester, M13 9PL, Manchester, UK
dc.contributorSchool of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham, B15 2TT, UK
dc.contributorAstrophysics Group, Leonard-Jones Building, Keele University, Staffordshire, ST5 5BG, UK
dc.contributorDepartment of Physical Sciences, The Open University, Walton Hall, Milton Keynes, MK7 6AA, UK
dc.contributorDominion Radio Astrophysical Observatory, National Research Council Canada, PO Box 248, Penticton, BC V2A 6J9, Canada; ALMA, Alonso Cordoba 3107, 7630355, Vitacura, Chile
dc.contributorSchool of Physics and Astronomy, E. C. Stoner Building, The University of Leeds, Leeds, LS2 9JT, UK
dc.contributorArmagh Observatory, College Hill, Armagh, BT61 9DG, Northern Ireland, UK
dc.contributor.authorMorford, J. C.
dc.contributor.authorFenech, D. M.
dc.contributor.authorPrinja, R. K.
dc.contributor.authorBlomme, R.
dc.contributor.authorYates, J. A.
dc.contributor.authorDrake, J. J.
dc.contributor.authorEyres, S. P. S.
dc.contributor.authorRichards, A. M. S.
dc.contributor.authorStevens, I. R.
dc.contributor.authorWright, N. J.
dc.contributor.authorClark, J. S.
dc.contributor.authorDougherty, S.
dc.contributor.authorPittard, J. M.
dc.contributor.authorSmith, H. A.
dc.contributor.authorVink, J. S.
dc.date.accessioned2024-02-21T11:03:35Z
dc.date.available2024-02-21T11:03:35Z
dc.date.issued2020-05-01T00:00:00Z
dc.identifier.doi10.1051/0004-6361/201731379
dc.identifier.doi10.48550/arXiv.2001.06363
dc.identifier.other2020arXiv200106363M
dc.identifier.otherastro-ph.SR
dc.identifier.otherastro-ph.GA
dc.identifier.other10.48550/arXiv.2001.06363
dc.identifier.other2020A&A...637A..64M
dc.identifier.other2020arXiv200106363M
dc.identifier.otherarXiv:2001.06363
dc.identifier.other10.1051/0004-6361/201731379
dc.identifier.other-
dc.identifier.other0000-0001-8443-1649
dc.identifier.urihttp://hdl.handle.net/20.500.14302/1882
dc.description.abstractContext. The role of massive stars is central to an understanding of galactic ecology. It is important to establish the details of how massive stars provide radiative, chemical, and mechanical feedback in galaxies. Central to these issues is an understanding of the evolution of massive stars, and the critical role of mass loss via strongly structured winds and stellar binarity. Ultimately, and acting collectively, massive stellar clusters shape the structure and energetics of galaxies. <BR /> Aims: We aim to conduct high-resolution, deep field mapping at 21 cm of the core of the massive Cygnus OB2 association and to characterise the properties of the massive stars and colliding winds at this waveband. <BR /> Methods: We used seven stations of the e-MERLIN radio facility, with its upgraded bandwidth and enhanced sensitivity to conduct a 21 cm census of Cygnus OB2. Based on 42 hours of observations, seven overlapping pointings were employed over multiple epochs during 2014 resulting in 1σ sensitivities down to ∼21 μJy and a resolution of ∼180 mas. <BR /> Results: A total of 61 sources are detected at 21 cm over a ∼0.48° × 0.48° region centred on the heart of the Cyg OB2 association. Of these 61 sources, 33 are detected for the first time. We detect a number of previously identified sources including four massive stellar binary systems, two YSOs, and several known X-ray and radio sources. We also detect the LBV candidate (possible binary system) and blue hypergiant star of Cyg OB2 #12. <BR /> Conclusions: The 21 cm observations secured in the COBRaS Legacy project provide data to constrain conditions in the outer wind regions of massive stars; determine the non-thermal properties of massive interacting binaries; examine evidence for transient sources, including those associated with young stellar objects; and provide unidentified sources that merit follow-up observations. The 21 cm data are of lasting value and will serve in combination with other key surveys of Cyg OB2, including Chandra and Spitzer.
dc.publisherAstronomy and Astrophysics
dc.titleCOBRaS: The e-MERLIN 21 cm Legacy survey of Cygnus OB2
dc.typearticle
dc.source.journalA&A
dc.source.journalA&A...637
dc.source.volume637
refterms.dateFOA2024-02-21T11:03:35Z
dc.identifier.bibcode2020A&A...637A..64M


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