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19 April 2024
 
  » arxiv » 0711.4038

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Spitzer IRS Spectra and Envelope Models of Class I Protostars in Taurus
E. Furlan ; M. McClure ; N. Calvet ; L. Hartmann ; P. D'Alessio ; W. J. Forrest ; D. M. Watson ; K. I. Uchida ; B. Sargent ; J. D. Green ; T. L. Herter ;
Date 26 Nov 2007
AbstractWe present Spitzer Infrared Spectrograph spectra of 28 Class I protostars in the Taurus star-forming region. The 5 to 36 micron spectra reveal excess emission from the inner regions of the envelope and accretion disk surrounding these predecessors of low-mass stars, as well as absorption features due to silicates and ices. Together with shorter- and longer-wavelength data from the literature, we construct spectral energy distributions and fit envelope models to 22 protostars of our sample, most of which are well-constrained due to the availability of the IRS spectra. We infer that the envelopes of the Class I objects in our sample cover a wide range in parameter space, particularly in density and centrifugal radius, implying different initial conditions for the collapse of protostellar cores.
Source arXiv, 0711.4038
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