Numerical simulations of the formation of protostellar discs.

Details Numerical simulations of the formation of protostellar discs. Numerical simulations of the formation of protostellar discs.

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992dudi.work..118p&link_type=abstract

"Dusty Discs, Proceedings of the 9th RAL Workshop on Astronomy and Astrophysics. Edited by P.M. Gondhalekar.

Astronomy and Astrophysics

Astrophysics

Scientific paper

The authors report the results of the first computer simulations capable of following the condensation of protostars out of turbulent interstellar gases. These protostars are rotationally supported discs with masses in the range 2 - 20 Msun and diameters from 100 - 4000 AU. In many of the simulations multiple protostellar systems were formed.

Affiliated with

Also associated with

No associations

Rating

Numerical simulations of the formation of protostellar discs. does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Numerical simulations of the formation of protostellar discs., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Numerical simulations of the formation of protostellar discs. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1114268