Exploring Asymmetries in Circumstellar Environments: Winds, Disks, and Things That Go Clump in the Light

Details Exploring Asymmetries in Circumstellar Environments: Winds, Disks, and Things That Go Clump in the Light Exploring Asymmetries in Circumstellar Environments: Winds, Disks, and Things That Go Clump in the Light

Feb 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002stin...0229622w&link_type=abstract

Technical Report, Smithsonian Astrophysical Observatory Cambridge, MA United States

Astronomy and Astrophysics

Astrophysics

Monte Carlo Method, Radiative Transfer, Data Processing, Star Formation, Stellar Winds, Stellar Envelopes, Stellar Systems, Coronal Loops

Scientific paper

The aim of the NASA LTSA Grant NAG5-6039 was to develop Monte Carlo radiation transfer techniques for use in the analysis of data from stellar systems that exhibit evidence for extended, non-spherical circumstellar environments. The broad applicability of the codes I have developed has opened many new research areas to me, as is reflected by the range of topics covered in the bibliography.

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