A radial velocity survey of the H II region S101

Details A radial velocity survey of the H II region S101 A radial velocity survey of the H II region S101

Oct 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982ap%26ss..87...13j&link_type=abstract

Astrophysics and Space Science, vol. 87, no. 1-2, Oct. 1982, p. 13-20. Research sponsored by the Science Research Council.

Computer Science

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Astronomical Models, H Ii Regions, Photoionization, Radial Velocity, Stellar Evolution, Computer Graphics, Stellar Temperature

Scientific paper

A pressure-scanned Fabry-Perot polychromator/imager has been used to conduct a radial velocity survey of the H II region S101. A tentative model of S101 is proposed, in light of a discussion of observation results, in which the H II/H I molecular comoving sheets furnish a useful way of describing the dynamics of H II regions generally. The existing dynamical structure is revealed by photoionization, rather than being generated by the interaction of the star with its surroundings.

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