The cobwebs of Ophiuchus. I - Strands of (C-13)O - The mass distribution

Details The cobwebs of Ophiuchus. I - Strands of (C-13)O - The mass distribution The cobwebs of Ophiuchus. I - Strands of (C-13)O - The mass distribution

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...338..902l&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 338, March 15, 1989, p. 902-924.

Astronomy and Astrophysics

Astrophysics

239

Carbon Monoxide, Interstellar Chemistry, Molecular Clouds, Nebulae, Ophiuchi Clouds, Carbon Isotopes, Frequency Distribution, Magnetic Fields, Mass Distribution, Spatial Distribution, Star Formation, Temperature Distribution

Scientific paper

A 4.5 deg x 6.5 deg area of the Rho Ophiuchus molecular complex has been mapped in J = 1-0 (C-13)O with a 2.4 arcmin beam. The spatial distribution of (C-13)O, the distribution of clumps according to size, mass, density, and kinetic temperature are described. The distribution of material in the cloud is compared with the magnetic field distribution and with a shocked cloud model. Evidence supporting the role of shock in the cloud is found in the cloud morphology.

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