Infrared Radiation Associated with Protostars

Details Infrared Radiation Associated with Protostars Infrared Radiation Associated with Protostars

Apr 1969

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1969rspta.264..227c&link_type=abstract

Philosophical Transactions for the Royal Society of London. Series A, Mathematical and Physical Sciences, Volume 264, Issue 1150

Physics

Scientific paper

Various stages in the collapse of an interstellar gas cloud into a cluster of protostars are discussed. The residual gas of the cloud which does not go into the protostars should form an opaque envelope which will thermalize the energy output of the protostars and be detectable as a high-luminosity infrared object. The infrared object in Orion newly discovered by Low is interpreted to be one of these objects.

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