Constraints on Nebular Dynamics Based on Observations of Annealed Magnesium Silicate Grains in Comets and in Disks Around Herbig AE and Be Stars

Details Constraints on Nebular Dynamics Based on Observations of Annealed Magnesium Silicate Grains in Comets and in Disks Around Herbig AE and Be Stars Constraints on Nebular Dynamics Based on Observations of Annealed Magnesium Silicate Grains in Comets and in Disks Around Herbig AE and Be Stars

Mar 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999lpi....30.1726n&link_type=abstract

30th Annual Lunar and Planetary Science Conference, March 15-29, 1999, Houston, TX, abstract no. 1726

Physics

15

Scientific paper

Observations of "crystalline olivine" grains in comets and in the disks
surrounding Herbig Ae & Be stars indicate the action of a continuous
flow of material from the inner to the outer regions of protoplanetary
nebulae not accounted for in current nebular models.

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