Analysis of obscured infrared point sources. V - S106 IR and S235 B

Details Analysis of obscured infrared point sources. V - S106 IR and S235 B Analysis of obscured infrared point sources. V - S106 IR and S235 B

Oct 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979apj...233..127t&link_type=abstract

Astrophysical Journal, Part 1, vol. 233, Oct. 1, 1979, p. 127-131.

Astronomy and Astrophysics

Astronomy

47

Infrared Astronomy, Point Sources, Protostars, Stellar Evolution, B Stars, H Ii Regions, Main Sequence Stars, O Stars, Stellar Models

Scientific paper

Moderate-resolution spectra of S106 IR and S235 B at 2 microns are presented. Strong B-gamma emission is observed in both sources. A simple model consisting of a zero-age main-sequence star (ZAMS) surrounded by a compact H II region is proposed for both sources. It is found that the observed B-gamma fluxes are consistent with ZAMS spectral types of O7.5 and B0 for S106 IR and S235 B, respectively.

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