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The Near-ultraviolet Spectra of FU Orionis Accretion Disks

  • Authors: Adolfo S. Carvalho, Lynne A. Hillenbrand, Gregory J. Herczeg, Kevin France

Adolfo S. Carvalho et al 2025 The Astrophysical Journal Letters 994 .

  • Provider: AAS Journals

Caption: Figure A1.

The 2D rectified x2d HST/STIS images for each of our sources. The white hashes mark the locations of the C II] 2326, Fe II] 2500, and Mg II 2800 features, and the surface brightness units are 10−14 erg s−1 cm−2 Å−1 arcsec−2. Notice that the traces of FU Ori, V1515 Cyg, and V960 Mon are all detected down to 1800 Å. BBW 76 is only marginally detected at 2100 Å. V1057 Cyg is only detected redward of the C II feature, with barely any continuum until 2400 Å, and HBC 722 is only detected redward of 2450 Å.

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