Physical characteristics of young star formation region ON1

Details Physical characteristics of young star formation region ON1 Physical characteristics of young star formation region ON1

Sep 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988sssmp..31.1116z&link_type=abstract

Scientia Sinica, Series A - Mathematical, Physical, Astronomical and Technical Sciences (ISSN 0253-5831), vol. 31, Sept. 1988, p

Physics

B Stars, Early Stars, H Ii Regions, Star Formation, Stellar Physics, Electron Density (Concentration), Gas Ionization, Physical Properties, Stellar Mass, Very Large Array (Vla)

Scientific paper

The paper reports VLA observations of the ON1 continuum radiation at 1.3-cm and 2-cm wavelengths. The physical parameters of the HII region ON1 are derived using a shell structure model. The inner and outer radii and the distribution function of the electron density are calculated from the continuum spectrum of ON1, and the results are found to be consistent with the observational data. It is suggested that the analysis of the continuum spectrum may provide a method to obtain the geometry of the HII region.

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