Star formation in IC 1848 A

Details Star formation in IC 1848 A Star formation in IC 1848 A

Dec 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...242..609t&link_type=abstract

Astrophysical Journal, Part 1, vol. 242, Dec. 1, 1980, p. 609-614.

Astronomy and Astrophysics

Astrophysics

16

Infrared Stars, Molecular Clouds, Nebulae, Star Formation, Stellar Spectra, H Ii Regions, Infrared Spectra, Stellar Models, Stellar Spectrophotometry

Scientific paper

Recent far-infrared photometric and near-infrared spectroscopic observations of IC 1848 A/W5 East are reported. The source appears to be excited by a star of spectral type near B0, which can explain the far-infrared luminosity, 2 micron spectrum, radio continuum, and radio molecular observations. Although this star appears surrounded by a local very compact H II region, the density over a large scale is relatively low. This puts constraints on models for the formation of this star.

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