Discovery of the first methanol (CH3OH) maser in the Andromeda galaxy (M31)

37Citations
Citations of this article
16Readers
Mendeley users who have this article in their library.

Abstract

We present the first detection of a 6.7 GHz Class II methanol (CH 3OH) maser in the Andromeda galaxy (M31). The CH3OH maser was found in a VLA survey during the fall of 2009. We have confirmed the methanol maser with the new EVLA, in operation since 2010 March, but were unsuccessful in detecting a water maser at this location. A direct application for this methanol maser is the determination of the proper motion ofM31, such as was previously obtained with water masers in M33 and IC10. Unraveling the three-dimensional velocity of M31 would solve for the biggest unknown in the modeling of the dynamics and evolution of the Local Group of galaxies. © 2010 The American Astronomical Society. All rights reserved.

Cite

CITATION STYLE

APA

Sjouwerman, L. O., Murray, C. E., Pihlström, Y. M., Fish, V. L., & Araya, E. D. (2010). Discovery of the first methanol (CH3OH) maser in the Andromeda galaxy (M31). Astrophysical Journal Letters, 724(2 PART 2). https://doi.org/10.1088/2041-8205/724/2/L158

Register to see more suggestions

Mendeley helps you to discover research relevant for your work.

Already have an account?

Save time finding and organizing research with Mendeley

Sign up for free