Interstellar A-type methanol masers

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

4

Interstellar Masers, Methyl Alcohol, Organic Lasers, Radiative Transfer, Absorption Spectra, H Ii Regions, Histories, Molecular Clouds

Scientific paper

The formation conditions for A-type methanol masers are discussed. The correlation between A-type masers and external radiation fields is determined, with emphasis on the energy levels of A-type methanol and brightness temperature. Radiative transfer equations and statistical equilibrium are solved using a large velocity gradient model and the escape probability model. It is demonstrated that the 9(2)-10(1)A+ emission in W3(OH) and 7(0)-6(1)A in SgrB2 are masers, as discovered previously. The formation of the first type of masers requires pumping from an external radiation field, while the second type might be excited in the absence of an external radiation field. It is also pointed out that according to calculations there are A-type maser series similar to E-type methanol maser series of J2-J1E.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Interstellar A-type methanol masers 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 Interstellar A-type methanol masers, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Interstellar A-type methanol masers will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1841077

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.