We use cookies to distinguish you from other users and to provide you with a better experience on our websites. Close this message to accept cookies or find out how to manage your cookie settings.
Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.
I consider maser emission in the H2O spectral line λ = 1.35 cm from long-period variable stars. Some models for H2O maser variability are suggested.
Rudnitskij, G.M.1987, in Circumstellar Matter, Proceedings of the 122nd Symposium of the International Astronomical Union, Held in Heidelberg, Germany, F.R. 23-27 June 1986, Appenzeller, I . & Jordan, C., Dordrecht: Reidel, 267Google Scholar
Rudnitskij, G.M.1990, in Proceedings of the International Colloquium From Miras to Planetary Nebulae: Which Path for Stellar Evolution? Montpellier, France, September 4-7, 1989, Mennessier, M.O. & Omont, A., Gif sur Yvette: Editions Frontières, 268Google Scholar