Analysis of obscured infrared objects. II - Allen's infrared source in NGC 2264

Details Analysis of obscured infrared objects. II - Allen's infrared source in NGC 2264 Analysis of obscured infrared objects. II - Allen's infrared source in NGC 2264

Nov 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978apj...226..119t&link_type=abstract

Astrophysical Journal, Part 1, vol. 226, Nov. 15, 1978, p. 119-123.

Astronomy and Astrophysics

Astronomy

38

Infrared Astronomy, Infrared Spectra, Stellar Models, Disks (Shapes), H Ii Regions, Main Sequence Stars, Nebulae, Stellar Evolution, Stellar Luminosity, Stellar Mass Accretion, Supergiant Stars, Ultraviolet Radiation

Scientific paper

Infrared spectra between 2 and 2.5 microns have been taken of the strong infrared source in NGC 2264. A strong line due to B-gamma has been detected in emission which represents the first indication of an H II region associated with the infrared object. The strength of this line, along with previous optical, infrared, and radio measurements, is used to investigate various models for the infrared source. Models using standard stars as the ionizing source cannot account for all of the observations. A model with a viscous disk component which is consistent with the observations is introduced as a possible model

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