Dust disks around young stars in Orion

Details Dust disks around young stars in Orion Dust disks around young stars in Orion

Jun 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995azh....72..397t&link_type=abstract

Astronomicheskij Zhurnal, vol. 72, p. 397

Astronomy and Astrophysics

Astronomy

2

Orion Nebula, Early Stars, Cosmic Dust, Protoplanets, Star Formation Rate, Stellar Envelopes, Interstellar Gas, Planetary Systems

Scientific paper

Possible reasons for the appearance of gas and dust shells around young stars are considered. The most plausible reason is believed to be the formation of protoplanetary gas and dust disks around a sizeable proportion of young stars simultaneously with their birth. A theoretical estimate of the formation rate for planetary systems around low-mass stars was found to be close to the observed one: about 40 percent of the star-formation rate.

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