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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. 3.

The ﹩19^{\prime \prime }\times 21^{\prime \prime }﹩ broadband and narrowband masked images of the region showing the morphology of the elongated reflection nebulosity around ISO‐Cha I 192. These were taken through filters centered in the Brγ and 2.12 μm H2 lines and the 2.09 μm continuum, as well as the ﹩K_{s}﹩ band. In all panels, the normalized PSF, defined as that of the nearby star [CCE98] 40, was subtracted from ISO‐Cha I 192. The bright (black) spot represents [CCE98] 40, and the noisy (top right) and white (other panels) circles represent the residuals of the PSF subtraction at the position of ISO‐Cha I 192 (see § 3.2 for details). The scale and orientation (north at top, east to the left) are identical for the six panels. The distance between ISO‐Cha I 192 and [CCE98] 40 is 10﹩\arcsec﹩.

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