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OH in Messier 82

2004/12/30 by M. K. Argo, A. Pedlar, Argo, M. K. +14
Engineering · Physics and Astronomy · #Astronomical Observations and Instrumentation #Astrophysical Phenomena and Observations #Calibration and Measurement Techniques #astro-ph

paper · pdf · doi:10.48550/arxiv.astro-ph/0412673

2 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

arxiv created 2004/12/30 · arxiv updated 2009/12/01

Abstract

Several 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.

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