An Accessible Model of Dynamics and Cycle for Interstellar OH and H2O Maser Associations

Details An Accessible Model of Dynamics and Cycle for Interstellar OH and H2O Maser Associations An Accessible Model of Dynamics and Cycle for Interstellar OH and H2O Maser Associations

Jan 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004ap%26ss.289..147l&link_type=abstract

Astrophysics and Space Science, v. 289, Issue 1, p. 147-160 (2004).

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

An accessible model for interstellar OH/H2O maser associations is presented. It can be classified into radiative pumping model. It can close the dynamical cycle of H2O and OH species, and can give an interpretation on interstellar OH/H2O associations. A reasonable scheme for both regeneration and destruction of interstellar H2O and OH molecules is argued. Our model has overcome the defects of former radiative models, and is compatible with astronomical conditions. It is shown that the rotational population of H2O and OH in these regions is much less affected by collisions than by radiation. Some experiments have confirmed our proposal.

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