Clumpy disk accretion and chondrule formation

Details Clumpy disk accretion and chondrule formation Clumpy disk accretion and chondrule formation

Nov 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993icar..106..168b&link_type=abstract

Icarus, vol. 106, p. 168

Physics

37

Accretion Disks, Chondrule, Early Stars, Clumps, Meteorites, Optical Thickness

Scientific paper

It is suggested that the source of the shocks whose induced heating may have been responsible for chrondrule formation was episodic accretion of low-mass clumps of interstellar gas onto the solar nebula. These clumps may have arisen from the inhomogeneous infall of the residual molecular cloud core, or from the return of matter ejected from the stellar wind, or perhaps from a combination of these two effects. Infalling clumps impact the protoplanetary disk at high velocity, generating the intense heat required for chondrule formation.

Affiliated with

Also associated with

No associations

Rating

Clumpy disk accretion and chondrule formation 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 Clumpy disk accretion and chondrule formation, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Clumpy disk accretion and chondrule formation will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-810735