Physics
Scientific paper
Jan 1997
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997cokon.100..231k&link_type=abstract
Communications of the Konkoly Observatory, No. 100 (Vol. XII, 2), p. 231-238 (1997)
Physics
Scientific paper
The basic physics of astrophysical masers is briefly reviewed. First, a qualitative discussion of the basic concepts about masers is given. These are: amplification, saturation, thermalization, beaming, variability, spectra and line widths. The difference between laboratory and astrophysical masers is then discussed, the basic requirements for the construction of a maser model are presented and the accuracy with which the various inputs are known is commented on. A qualitative discussion is given of the most common models, which are collisional and radiative. The use of OH masers as diagnostics of physical conditions in star-forming regions is discussed in the end.
Kylafis Nick D.
Pavlakis Konstantinos G.
No associations
LandOfFree
Astrophysiscal 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 Astrophysiscal Masers in Star-Forming Regions, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Astrophysiscal Masers in Star-Forming Regions will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1786801