IRAS observations of the Rosette nebula complex

Details IRAS observations of the Rosette nebula complex IRAS observations of the Rosette nebula complex

Apr 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26a...230..181c&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 230, no. 1, April 1990, p. 181-192.

Astronomy and Astrophysics

Astronomy

61

H Ii Regions, Infrared Astronomy, Molecular Clouds, Nebulae, Carbon Monoxide, Infrared Astronomy Satellite, Star Formation

Scientific paper

A detailed study of the infrared radiation associated with the Rosette nebula complex has been conducted using the IRAS data. The results of the study suggest that most of the infrared sources detected by IRAS which are embedded in the Rosette molecular cloud are associated with dense molecular clumps. The luminosities of these sources cover the range 100-12,000 solar luminosities, corresponding to B1-B4 stellar types.

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