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Detection of Extended Thermal Infrared Emission around the Vega‐like Source HD 141569

  • Authors: R. S. Fisher, C. M. Telesco, R. K. Piña, R. F. Knacke, and M. C. Wyatt

Fisher et al. 2000 The Astrophysical Journal Letters 532 L141.

  • Provider: AAS Journals

Caption: Fig. 1.

Scans through HD 41569 and the PSF star. In all plots, HD 141569 is the solid line, and the PSF star is the dashed line. A Gaussian fit to the HD 141569 data is shown as the dotted line. (a) Scan through the major axis (﹩\mathrm{P}\,.\mathrm{A}\,.=175^{\circ }﹩) of HD 141569 at 10.8 μm. (b) Scan through the minor axis of HD 141569 at 10.8 μm. (c) Major axis (﹩\mathrm{P}\,.\mathrm{A}\,.=175^{\circ }﹩) scan at 18.2 μm. (d) Minor axis scan at 18.2 μm.

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