(C-12)O (J=1-0) and (J=2-1) mapping of the Zeta Ophiuchi diffuse cloud

Details (C-12)O (J=1-0) and (J=2-1) mapping of the Zeta Ophiuchi diffuse cloud (C-12)O (J=1-0) and (J=2-1) mapping of the Zeta Ophiuchi diffuse cloud

Jul 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...219..279l&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 219, no. 1-2, July 1989, p. 279-285.

Astronomy and Astrophysics

Astronomy

24

Astronomical Maps, Carbon Monoxide, Interstellar Matter, Molecular Clouds, Radio Sources (Astronomy), Molecular Spectra, Radio Spectra, Space Commercialization

Scientific paper

A one-arcmin region surrounding Zeta Oph has been mapped in (C-12)O (J=2-1) and (J=1-0) with full sampling at angular resolutions of 12 arcsec and 23 arcsec, respectively. It is found that the CO emission comes from two components at V(LSR) = -0.8 and 0.4 km/s, with temperatures (on the scale defined by Kutner and Ulich, 1981) of 1.6 and 0.7 K, respectively, for the J=1-0 line. The density structure of these components is examined.

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