A model for the Becklin-Neugebauer infrared point source

Details A model for the Becklin-Neugebauer infrared point source A model for the Becklin-Neugebauer infrared point source

Apr 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982pazh....8..234k&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 8, Apr. 1982, p. 234-237.) Soviet Astronomy Letters, vol. 8, Mar.-Apr. 1982, p. 124-126

Astronomy and Astrophysics

Astronomy

1

Infrared Astronomy, Main Sequence Stars, Stellar Evolution, Stellar Models, Luminous Intensity, Molecular Clouds, Orion Nebula, Radiation Pressure, Stellar Envelopes

Scientific paper

The strong point source of IR radiation discovered by Becklin and Neugebauer in 1967, and named BN after them, is presently modeled as a massive star in formation. The radiation pressure of a star-like core of 14 solar masses and 10,000 solar luminosities is producing a dense shell near the dust sublimation radius within an extended gas-dust envelope, according to the new model.

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