Radio continuum and CO (J = 2 to 1) observations of NGC 3628

Details Radio continuum and CO (J = 2 to 1) observations of NGC 3628 Radio continuum and CO (J = 2 to 1) observations of NGC 3628

Aug 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26a...248...12r&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 248, no. 1, Aug. 1991, p. 12-22.

Astronomy and Astrophysics

Astrophysics

26

Carbon Monoxide, Interacting Galaxies, Molecular Clouds, Radio Emission, Starburst Galaxies, Astronomical Spectroscopy, Molecular Excitation, Molecular Gases, Very Large Array (Vla)

Scientific paper

The present 20-cm wavelength radio continuum emission observations of the (C-12)O and (C-13)O 2-1 lines in the edge-on galaxy NGC 3628 indicate a total molecular gas mass of 1.3 billion solar masses for the central 4 x 1 kpc of the galaxy. Only a small fraction of the molecular gas is concentrated in high density cores of the molecular clouds. Evidence is found for a spiral arm structure from both the radio continuum and the CO observations.

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