Microwave emission from stars.

Abstract

An attempt is made to summarize the observations of masered emission from stars and to outline some basic conclusions that can be drawn from the data. The association of masered microwave emission with well studied objects like stars makes it possible to use the information gathered by conventional optical observations to attack the general masering problem and, conversely, the radio observations may be used to obtain information about a star not readily accessible optically, such as the mass loss rate or the physical conditions in a circumstellar shell.