The Circumstellar Environment of Low Mass Star Forming Regions

Details The Circumstellar Environment of Low Mass Star Forming Regions The Circumstellar Environment of Low Mass Star Forming Regions

Jun 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997stin...9727089b&link_type=abstract

Technical Report, NASA-CR-204638; NAS 1.26:204638 Dept. of Terrestrial Magnetism

Computer Science

Stellar Envelopes, Spatial Resolution, Radiative Transfer, Millimeter Waves, Angular Resolution, Stellar Mass Accretion, Stellar Structure, Stellar Mass Ejection, Microwave Interferometers, Imaging Techniques, Collapse, Free Fall, Dust

Scientific paper

We have obtained the complete SED from 10 microns out to 1.3 mm for all
of our sources. We have the FIR imaging data, processed to reveal the
maximum angular resolution possible, which allows us to model the disk.
To model the disk, we have high resolution millimeter interferometry
data.

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