Astronomy and Astrophysics – Astrophysics
Scientific paper
Nov 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...346..983e&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 346, Nov. 15, 1989, p. 983-990.
Astronomy and Astrophysics
Astrophysics
230
Interstellar Masers, Star Formation, Water Masers, Abundance, Astronomical Models, Brightness Temperature, Emission Spectra, Maser Pumping, Shock Waves
Scientific paper
A comprehensive model is presented for the powerful H2O masers observed in star-forming regions. The shocks are the result of interaction of dense, high-velocity clumps with dense shells or clumps in the ambient medium. The shocked material is a thin slab in physical space, but breaks up into a network of filaments in velocity space. These filaments are the individual H2O maser features. The results of maser model calculations are presented which provide the maximum brightness temperatures that can be produced in single-temperature environments of any kind.
Elitzur Moshe
Hollenbach David J.
McKee Christopher F.
No associations
LandOfFree
H2O masers in star-forming regions does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with H2O masers in star-forming regions, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and H2O masers in star-forming regions will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1613816