The Λ0 = 1.35 cm H2O maser line: The hyperfine structure and profile asymmetry

Details The Λ0 = 1.35 cm H2O maser line: The hyperfine structure and profile asymmetry The Λ0 = 1.35 cm H2O maser line: The hyperfine structure and profile asymmetry

Jan 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006astl...32...29v&link_type=abstract

Astronomy Letters, vol. 32, Issue 1, p.29-38

Astronomy and Astrophysics

Astronomy

5

Pacs Numbers 98.58.Ec

Scientific paper

The spectra of several H2O maser sources exhibit single λ0 = 1.35 cm maser lines with narrow asymmetric profiles. We consider the hyperfine structure of the line that corresponds to the transition between the rotational 616 → 523 levels of ortho-H2O molecules to account for the line asymmetry. Our numerical simulations of the maser line profile agree well with the observations if the hyperfine structure is taken into account.

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