Modelling Far-Infrared Observations of Young Stellar Objects

Details Modelling Far-Infrared Observations of Young Stellar Objects Modelling Far-Infrared Observations of Young Stellar Objects

Feb 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ap%26ss.224...77b&link_type=abstract

Astrophysics and Space Science, Volume 224, Issue 1-2, pp. 77-80

Astronomy and Astrophysics

Astrophysics

2

Star Formation:Theory, Far Infrared:Observations, Radiative Transport:Models, Young Stellar Objects:Taurus

Scientific paper

We discuss high-resolution, far-infrared spatial observations of low mass embedded young stellar objects in the Taurus molecular complex. By comparing the observed spatial extent with the results of radiative transport models, we can estimate the density distribution of the envelopes. We compare the initial results for 4 objects (L1551-IRS 5, L1489-IR, L1551-NE, and L1527-IR) with star formation theories.

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