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Spitzer IRS Spectra and Envelope Models of Class I Protostars in Taurus

  • Authors: 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, and T. L. Herter

Furlan et al. 2008 The Astrophysical Journal Supplement Series 176 184.

  • Provider: AAS Journals

Caption: Fig. 3.

SED plots of the Class I objects in our sample, ordered alphabetically by their name. Optical to mid‐IR, ground‐based photometry is shown as filled diamonds, the 2MASS J, H, and Ks fluxes as filled circles, the IRAC 3.6, 4.5, 5.8, and 8.0 μm fluxes as open circles, the IRAS 12, 25, and 60 μm fluxes as open diamonds or open triangles, if upper limits, and submillimeter and millimeter fluxes, where available, as filled squares. The IRS spectrum is also shown. No corrections for reddening have been applied.

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