Spectral and isophotal appearance of three-dimensional protostellar models

Details Spectral and isophotal appearance of three-dimensional protostellar models Spectral and isophotal appearance of three-dimensional protostellar models

Apr 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apj...353..236b&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 353, April 10, 1990, p. 236-244.

Astronomy and Astrophysics

Astronomy

14

Astronomical Models, Protostars, Stellar Evolution, Infrared Astronomy Satellite, Radiative Transfer, Stellar Spectra, Temperature Distribution

Scientific paper

The first 'self-consistent' models of the spectral and isophotal appearance of fully three-dimensional models of protostellar formation are presented. The spectra show that the emission for these models peaks in the submillimeter range, with the spectra typically resembling those of 10 K blackbodies. Although their spectra may be similar, binary protostellar clouds can be distinguished from single protostellar cloud through their binary isophotal appearance, providing the beam size is sufficiently small and the viewing angle is favorable.

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