CS, C(3)S(4), and CH3OH observations of the molecular cloud associated with NGC 7538

Details CS, C(3)S(4), and CH3OH observations of the molecular cloud associated with NGC 7538 CS, C(3)S(4), and CH3OH observations of the molecular cloud associated with NGC 7538

Jan 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ap%26ss.118..449k&link_type=abstract

(IAU, Asian-Pacific Regional Meeting, 3rd, Kyoto, Japan, Sept. 30-Oct. 5, 1984) Astrophysics and Space Science (ISSN 0004-640X),

Astronomy and Astrophysics

Astrophysics

Emission Spectra, Molecular Clouds, Molecular Spectra, Carbon Compounds, Methyl Alcohol, Sulfides

Scientific paper

CS(J = 1-0), C34S(J = 1-0), and CH3OH(10-00 A and E) emission lines in the core region of the molecular cloud associated with NGC 7538 have been surveyed at angular resolution of 33arcsec. Distribution of CS column density shows two prominent peaks. Both blue and red wings in CS line are most prominent at 30arcsec northwest of IRS 11.

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