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ISO‐Cha I 192: A New Embedded Eruptive Variable in the Chamaeleon I Dark Cloud

  • Authors: P. Persi, M. Tapia, M. Gòmez, B. A. Whitney, A. R. Marenzi, and M. Roth

Persi et al. 2007 The Astronomical Journal 133 1690.

  • Provider: AAS Journals

Caption: Fig. 4.

Observed 2003–2004 SED of ISO‐Cha I 192. The solid line represents the best fit of the disk + envelope model (see text). The errors are estimated to be similar to the size of the symbols, except those derived from the spectrum by Pontoppidan et al. (2003; pentagons), which are estimated to be larger.

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