BN objects - A class of very young and massive stars

Details BN objects - A class of very young and massive stars BN objects - A class of very young and massive stars

Dec 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ap%26ss.128..199h&link_type=abstract

(Universitaets-Sternwarte Jena, Jena Workshop on the Role of Dust in Dense Regions of Interstellar Matter, Georgenthal, East Ger

Astronomy and Astrophysics

Astrophysics

10

Infrared Stars, Protostars, Stellar Envelopes, Stellar Evolution, Supermassive Stars, Absorption Spectra, H Ii Regions, Stellar Spectra, Stellar Structure, Stellar Winds

Scientific paper

The Becklin-Neugebauer objects are identified by means of a wide range of observable features as a separate class of very young and massive stars surrounded by optically thick dust shells. The authors show that they evolutionarily connect real protostars to compact H II regions. They give criteria which should be appropriate to segregate the BN objects from compact H II regions. Finally, they describe the structure of a typical BN object.

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