Statistics – Computation
Scientific paper
Sep 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987apj...320..258s&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 320, Sept. 1, 1987, p. 258-265.
Statistics
Computation
24
Cosmic Dust, Infrared Sources (Astronomy), Interstellar Gas, Stellar Evolution, Stellar Winds, Supernovae, Computational Astrophysics, H I Regions, H Ii Regions, Infrared Astronomy Satellite, Interstellar Matter
Scientific paper
Loops containing diffuse and discrete emission are a feature of the IRAS sky images. Some of these loops are limb-brightened shells resulting from supernovae or stellar winds acting on the interstellar medium. Secondary star formation appears to have occurred at the surface of these shells. A significant proportion of the early-type stars in the solar neighborhood appear to have formed in stellar loops.
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