Methanol maser groups and class I emission: Flux density distribution

Details Methanol maser groups and class I emission: Flux density distribution Methanol maser groups and class I emission: Flux density distribution

Oct 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007arep...51..813l&link_type=abstract

Astronomy Reports, Volume 51, Issue 10, pp.813-819

Astronomy and Astrophysics

Astronomy

98.58.Ec

Scientific paper

A search for a relationship between class I and class II methanol maser flux densities has been carried out. A large sample of mixed-type sources has been studied, with each source in the sample radiating as a class I and class II maser simultaneously. In methanol maser groups for which the positions of prominent spectral features at different radial velocities coincide at different frequencies, the fluxes are anticorrelated, and are related as log S 6.7+12.2 = (-1.68 ± 0.38) × log S 44 + (4.01 ± 0.60). For group I, which includes sources with preferred pumping for masers emitting at 6.7 GHz, the relationship between the 6.7 GHz masers and 44 GHz masers is less steep than for group II, which contains sources with normal pumping of class II masers. This implies that class I methanol masers that correspond to group I are suppressed more strongly.

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