Fig. 6 from Spitzer IRS Spectra and Envelope Models of Class I Protostars in Taurus

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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. 6.

IRS spectra of both components of the 21^{﹩\arcsec﹩} binary IRAS 04108+2803, plotted on the same scale. While observing 04108+2803A, the bright B component partly entered the LL slit, and therefore, the spectrum of component A beyond 14 μm contains an increasing amount of emission from component B; the spectrum of A is dominated by emission from B beyond about 20 μm.

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