Fine structure in H II regions. II

Details Fine structure in H II regions. II Fine structure in H II regions. II

Dec 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974apj...194..279t&link_type=abstract

Astrophysical Journal, vol. 194, Dec. 1, 1974, pt. 1, p. 279-291.

Astronomy and Astrophysics

Astronomy

63

Astronomical Maps, Fine Structure, H Ii Regions, Interstellar Gas, Microwave Emission, Radio Astronomy, Emission Spectra, Hydrogen Ions, Hydroxyl Emission, Infrared Astronomy, Ionized Gases, Microwave Interferometers, Spectral Emission

Scientific paper

Interferometric synthesis of the continuum emission at 11-cm wavelength has been performed for several galactic H II regions which lie near sources of O H and H2O emission. The spatial resolution is between 4.9 and 17.2 sec in the narrowest direction. Fine structure with scales sizes of order 0.1 pc are observed in some cases, where intermediate (about 3 pc) or no small structure is found in others. The relationship of the continuum structure to the distribution of molecules such as CO, CS, and HCN, to the positions of OH and H2O emission, and to preliminary maps in the infrared is discussed. A qualitative picture which is consistent with these relationships is developed.

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