OH in Messier 82

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dc.creatorArgo, M. K.
dc.creatorPedlar, A.
dc.creatorMuxlow, T. W. B.
dc.creatorBeswick, R. J.
dc.creatorAalto, S.
dc.creatorWills, K.
dc.creatorBooth, R.
dc.date2004-12-30
dc.date.accessioned2026-07-07T02:16:30Z
dc.date.available2026-07-07T02:16:30Z
dc.descriptionSeveral new main line OH masers have been detected in the nearby starburst galaxy M82. Eight masers have been detected to 5 sigma, six of which are new detections. Observations covering both the 1665 and 1667 MHz lines with both the Very Large Array (VLA) and the Multi-Element Radio Linked Interferometer Network (MERLIN) have been used to accurately measure the positions and velocities of these features. Following analysis of the data, another six objects below 5 sigma, but with velocities consistent with the distribution inferred from the more certain detections, have been detected. These are classified as possible detections.
dc.description2 pages. 2 figures. Proceedings of the 7th European VLBI Network Symposium held in Toledo, Spain on October 12-15, 2004. Editors: R. Bachiller, F. Colomer, J.-F. Desmurs, P. de Vicente (Observatorio Astronomico Nacional), p. 151-152. Needs evn2004.cls
dc.identifierhttps://arxiv.org/abs/astro-ph/0412673
dc.identifierhttp://arxiv.org/abs/astro-ph/0412673
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/8811
dc.subjectAstrophysics
dc.titleOH in Messier 82
dc.typetext

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