Two-stage fragmentation in a rotating protostellar cloud

Details Two-stage fragmentation in a rotating protostellar cloud Two-stage fragmentation in a rotating protostellar cloud

Aug 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979ap%26ss..64..463p&link_type=abstract

Astrophysics and Space Science, vol. 64, no. 2, Aug. 1979, p. 463-466. Research sponsored by the Consiglio Nazionale Delle Rice

Computer Science

Numerical Analysis

1

Protostars, Stellar Models, Stellar Rotation, Stellar Structure, Fragmentation, Numerical Analysis, Qualitative Analysis, Turbulence Effects

Scientific paper

The paper discusses the problem of fragmentation in a rotating cloud, showing that different physical models can result in widely different results. It is also shown that results of the present 'turbulent-rotation' model agree qualitatively with those of numerical calculations by Larson (1978) and it is suggested that fragmentation in a rotating nebula takes place at two different stages.

Affiliated with

Also associated with

No associations

Rating

Two-stage fragmentation in a rotating protostellar cloud 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 Two-stage fragmentation in a rotating protostellar cloud, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Two-stage fragmentation in a rotating protostellar cloud will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1483478