Disk Chemistry and Cometary Composition

Details Disk Chemistry and Cometary Composition Disk Chemistry and Cometary Composition

May 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003dps....35.2806m&link_type=abstract

American Astronomical Society, DPS meeting #35, #28.06; Bulletin of the American Astronomical Society, Vol. 35, p.968

Astronomy and Astrophysics

Astrophysics

Scientific paper

We will describe current chemical modelling of disks similar to the protosolar nebula. Calculations are being undertaken to determine the spatial and temporal chemistry of the gas and dust within the 5-40AU comet-forming region of the nebula. These theoretical studies aim to determine the contribution of pristine and partially-processed interstellar material from the cool outer nebula, as compared to that obtained from outward radial mixing of matter from the hot inner nebula.
Reference Molecular distributions in the inner regions of protostellar disks, Markwick, A. J., Ilgner, M., Millar, T. J., Henning, Th. (2002), Astron. Astrophys., 385, 632.

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