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- W2034379927 abstract "view Abstract Citations (61) References (25) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS Disk structure in protostellar H2O maser sources. Elmegreen, B. G. ; Morris, M. Abstract Protostellar maser sources are modeled as orbiting gaseous disks surrounding massive windy stars. According to the model, parts of the disk may be H2O masers. The high-velocity features seen in several H2O sources may be due to the material ejected from the inner regions of the disk by pressure from the wind. Radial intervals in which the gas density is suitable for a maser determine the velocity and distance range of these features. Maser spot size, the temperatures and densities in the maser region, and the duration of the maser phase can all be accounted for through reference to the model. Publication: The Astrophysical Journal Pub Date: April 1979 DOI: 10.1086/156994 Bibcode: 1979ApJ...229..593E Keywords: Interstellar Masers; Protostars; Stellar Models; Stellar Structure; Stellar Winds; Water Masers; Infrared Astronomy; Kelvin-Helmholtz Instability; Kepler Laws; Stellar Atmospheres; Stellar Envelopes; Stellar Evolution; Stellar Radiation; Astrophysics; Star Formation:Water Masers full text sources ADS |" @default.
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- W2034379927 date "1979-04-01" @default.
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- W2034379927 title "Disk structure in protostellar H2O maser sources" @default.
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