Modeling the Structure of Class I Young Stellar Objects

Details Modeling the Structure of Class I Young Stellar Objects Modeling the Structure of Class I Young Stellar Objects

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aas...20718513m&link_type=abstract

American Astronomical Society Meeting 207, #185.13; Bulletin of the American Astronomical Society, Vol. 37, p.1477

Astronomy and Astrophysics

Astronomy

Scientific paper

By using spectra taken with the Infrared Spectrograph (IRS) aboard the Spitzer Space Telescope, in conjunction with optical, near infrared, sub millimeter and radio data from ground based observations, we construct model spectral energy distributions (SEDs) for Class I Young Stellar Objects (YSOs) in Taurus. We use the SED to infer specific values for the parameters that describe the structure of the system, such as the size and shape of the envelope. We use our modeling code to create SEDs from 2 microns to 3 mm and match these models to our original spectrum and ancillary data, giving an interesting view of the structural evolution of Class I protostars.

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