Radio continuum interferometry of dark clouds. I - A search for newly formed H II regions.

Details Radio continuum interferometry of dark clouds. I - A search for newly formed H II regions. Radio continuum interferometry of dark clouds. I - A search for newly formed H II regions.

Jul 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980aj.....85..894g&link_type=abstract

Astronomical Journal, vol. 85, July 1980, p. 894-944.

Astronomy and Astrophysics

Astronomy

14

Continuous Spectra, H Ii Regions, Interferometry, Milky Way Galaxy, Physical Properties, Radio Astronomy, Astronomical Maps, Astronomical Models, Brightness Temperature, Galactic Structure, Light (Visible Radiation), Orion Constellation, Radio Spectra, Stellar Evolution, Tables (Data), Taurus Constellation

Scientific paper

The purpose of the study is to extend the knowledge of the categories of local objects by using a sensitive and thorough technique to identify which nearby dark molecular clouds are hiding newly formed massive stars. Investigations of the physical properties of some of the local regions of star formation are made in an effort to derive general properties of the local process(es) of massive star formation. Eleven H II regions with associated visible emission and 18 other sources identified as possible H II regions were detected. The individual regions of the star formations are studied in detail. The regions include S140 IR, S156, and Mon R2, as well as dark cloud complexes in Perseus, Taurus, Orion, and Ophiuchus. It is noted that local newly formed massive stars display predictable characteristics.

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