Observational Evidence for Very Large-scale Dust and Gas Transport in Protostellar Nebulae

Details Observational Evidence for Very Large-scale Dust and Gas Transport in Protostellar Nebulae Observational Evidence for Very Large-scale Dust and Gas Transport in Protostellar Nebulae

Mar 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002lpi....33.1247h&link_type=abstract

33rd Annual Lunar and Planetary Science Conference, March 11-15, 2002, Houston, Texas, abstract no.1247

Physics

3

Scientific paper

A vast transport system may have existed in the Solar nebula capable of
carrying great quantities of dust from the warm, inner nebula to beyond
the snowline. We are testing this hypothesis by observing winds around
nearby protoplanetary disk systems.

Affiliated with

Also associated with

No associations

Rating

Observational Evidence for Very Large-scale Dust and Gas Transport in Protostellar Nebulae 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 Observational Evidence for Very Large-scale Dust and Gas Transport in Protostellar Nebulae, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Observational Evidence for Very Large-scale Dust and Gas Transport in Protostellar Nebulae will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-785880