Hostname: page-component-78c5997874-fbnjt Total loading time: 0 Render date: 2024-11-14T06:58:50.383Z Has data issue: false hasContentIssue false
  • English
  • Français

Observations of variability of H2O Maser sources associated with star formation regions

Published online by Cambridge University Press:  03 August 2017

M. I. Pashchenko ,
E. E. Lekht ,
I. I. Berulis  and
R. L. Sorochenko
M. I. Pashchenko
Affiliation:
Sternberg State Astronomical Institute 13 Universitetskij prospect Moscow V-234, 119899 USSR
E. E. Lekht
Affiliation:
Sternberg State Astronomical Institute 13 Universitetskij prospect Moscow V-234, 119899 USSR
I. I. Berulis
Affiliation:
Lebedev Physics Institute, Academy of Sciences, Moscow
R. L. Sorochenko
Affiliation:
Lebedev Physics Institute, Academy of Sciences, Moscow

Abstract

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.

An outstanding feature of the water maser emission from star formation regions is the strong time variability, which was recognised soon after the discovery of interstellar H2O masers. It is likely that the observed considerable variations of the H2O line profiles as well as of the flux density reflect the disturbancies in the protostellar nebule probably associated with the outflow from the newly formed stars.

Type
Poster Sessions
Information
Symposium - International Astronomical Union , Volume 147: Fragmentation of Molecular Clouds and Star Formation , 1991 , pp. 482 - 484
Copyright
Copyright © Kluwer 1991 

References

Elmegreen, B. G. and Morris, M. (1979) Astrophys. J. 229, 593.Google Scholar
Berulis, I. I., Lekht, E. E., Pashchenko, M. I. (1987) Sov. Astron. Lett. 13(2), 124.Google Scholar