Evidence for the evolution of grain properties in the NGC 2024 star forming ridge.

Details Evidence for the evolution of grain properties in the NGC 2024 star forming ridge. Evidence for the evolution of grain properties in the NGC 2024 star forming ridge.

Oct 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996nascp3339..139c&link_type=abstract

Scientific conference: From stardust to planetesimals, p. 139 - 142

Physics

Star-Forming Regions: Dust Grains, Star-Forming Regions: Infrared Surveys, Interstellar Dust: Infrared Surveys

Scientific paper

High-resolution images of the NGC 2024 molecular ridge in CS(2-1) and 3
mm continuum emission have been obtained using the Owens Valley
millimeter array. The data are used to determine the temperature and
dynamics of the ridge, and to ascertain the evolutionary state of the
embedded protostars FIR2-7.

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