Study of CO in LYNDS 134

Details Study of CO in LYNDS 134 Study of CO in LYNDS 134

Jul 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976aj.....81..508m&link_type=abstract

Astronomical Journal, vol. 81, July 1976, p. 508-511.

Other

39

Astronomical Photography, Carbon Monoxide, Cosmic Dust, Molecular Excitation, Absorption Spectra, Luminous Intensity, Radial Velocity, Spectral Line Width, Telescopes

Scientific paper

Observations of C-12 0-16, C-13 0-16 and C-12 0-18 in the dark dust cloud Lynds 134 were made using with a 4.6 m telescope. There are four molecular clouds in the dust cloud, two of which, the most prominent, are approximately isothermal with an excitation temperature of about 12 K. A comparison of CO data with 21-cm line data indicates that these two clouds coincide in position, velocity, and linewidth with 21-cm absorption features.

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