2006Astronomy LettersRequires access

The λ0 = 1.35 cm H2O maser line: The hyperfine structure and profile asymmetry

Д. А. Варшалович, A. V. Ivanchik, N. S. Babkovskaya

Open publisher page 15 citations

Abstract

The spectra of several H 2 O maser sources exhibit single λ 0 = 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 6 16 → 5 23 levels of ortho-H 2 O 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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What this paper is about

The spectra of several H 2 O maser sources exhibit single λ 0 = 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 6 16 → 5 23 levels of ortho-H 2 O 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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Available abstract

The spectra of several H 2 O maser sources exhibit single λ 0 = 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 6 16 → 5 23 levels of ortho-H 2 O 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.

Key concepts: Maser, Hyperfine structure, Physics, Asymmetry, Line (geometry), Spectral line, Atomic physics, Astrophysics

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