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DJ van der Walt

On the periodic class II methanol masers in the high mass star forming region G9.62+0.20E

(Volume 80 - Année 2011)
Article
Open Access

Abstract

Class II methanol masers are known to be exclusively associated with high mass star forming regions. The phenomenon of periodic methanol masers associated with a small number of star forming regions is now known for a number of years. The underlying process(es) responsible for the periodicity is not known however. In this paper I present a simple colliding-wind scenario to try explain the periodicity and the flare profiles of the periodic flaring of the class II masers in the high-mass star forming region G9.62+0.02E. It is found that the 12.2 GHz methanol maser time series as well as the profiles of individual flares are reproduced very well under the assumption that the observed flaring is due to changes in the free-free background emission from the H II region. A number of other properties of the masers can also be explained within the framework of this model. It is concluded that a colliding-wind binary is a possible underlying cause for the periodic class II masers inG9.62+0.20E and should be investigated further.

Pour citer cet article

DJ van der Walt, «On the periodic class II methanol masers in the high mass star forming region G9.62+0.20E», Bulletin de la Société Royale des Sciences de Liège [En ligne], Volume 80 - Année 2011, 260 - 264 URL : https://popups.uliege.be/0037-9565/index.php?id=2734.

A propos de : DJ van der Walt

Centre for Space Research, North-West University, Potchefstroom, 2520, South Africa, johan.vanderwalt@nwu.ac.za