Active star formation in NGC 2264

Details Active star formation in NGC 2264 Active star formation in NGC 2264

May 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985apj...292..231s&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 292, May 1, 1985, p. 231-237.

Astronomy and Astrophysics

Astronomy

41

Early Stars, Infrared Astronomy, Molecular Clouds, Star Clusters, Star Formation, Stellar Spectrophotometry, Far Infrared Radiation, Gas Temperature, Molecular Spectra, Radio Sources (Astronomy)

Scientific paper

The region of NGC 2264 near the cone nebula is the site of active star
formation in a rotating ring seen nearly edge on as a two lobed source.
Allen's infrared source (IRS 1) surrounds a B3 V star still embedded in
the southern lobe of the cloud. The northern lobe, IRS 2, also probably
contains young stars.

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