Kinematics and morphology of material occulting Zeta Ophiuchi

Details Kinematics and morphology of material occulting Zeta Ophiuchi Kinematics and morphology of material occulting Zeta Ophiuchi

May 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992apj...390..226l&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 390, no. 1, May 1, 1992, p. 226-229.

Astronomy and Astrophysics

Astrophysics

10

Emission Spectra, Interstellar Matter, Molecular Clouds, Ophiuchi Clouds, Radio Spectra, Carbon Isotopes, Carbon Monoxide, Dynamics, Kinematics, Line Spectra, Morphology

Scientific paper

Attention is given to observations of 2.6-mm (C-12)O emission taken along a 2-deg strip about the position of Zeta Oph which show a strikingly coherent kinematic pattern. Within 30 arcmin of the star, (C-12)O line is as strong as 5.5 K, which is highly unusual. It is suggested that the CO line brightness is dominated by recombination and excitation effects in gas which is strongly affected by the presence of the star.

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