Detection of star formation regions near supernova remnant W44

Details Detection of star formation regions near supernova remnant W44 Detection of star formation regions near supernova remnant W44

Oct 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978m%26p....19..163w&link_type=abstract

(Conference on Protostars and Planets, Tucson, Ariz., Jan. 3-7, 1978.) Moon and the Planets, vol. 19, Oct. 1978, p. 163-168.

Computer Science

6

Hydrogen Clouds, Infrared Spectra, Protostars, Star Formation, Stellar Spectrophotometry, Supernova Remnants, Carbon Monoxide, Cosmology, Molecular Spectra, Radio Spectra, Stellar Luminosity

Scientific paper

Observations of two infrared objects embedded in molecular clouds near
the supernova remnant W44 are presented. W44-IRS1 offers compelling
evidence that it is a star whose formation was recently induced by
expansion of the supernova remnant. W44-IRS2 lies beyond the remnant,
possibly apart from the region of its influence.

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