Far-infrared observations of globules

Details Far-infrared observations of globules Far-infrared observations of globules

Apr 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981apj...245..115k&link_type=abstract

Astrophysical Journal, Part 1, vol. 245, Apr. 1, 1981, p. 115-123. Research supported by the Fannie and John Hertz Foundation;

Astronomy and Astrophysics

Astronomy

65

Cosmic Dust, Far Infrared Radiation, Infrared Astronomy, Interstellar Radiation, Molecular Clouds, Nebulae, Carbon Monoxide, Heat Sources, Infrared Spectra, Molecular Spectra, Spatial Distribution, Thermal Emission

Scientific paper

Observations of far-infrared emission from nine globules are presented. The intensity and uniformity of the emission confirm that the heat source is the interstellar radiation field. Spectra of B133 and B335 are presented; they are consistent with optically thin thermal emission from dust with temperature 13-16 K. The temperature and intensity of B335 are used to calculate the ratio of visual extinction to far-infrared emission frequency.

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