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Spectral Appearance of Self-gravitating Disks Powered by Stellar Objects: Universal Effective Temperature in the Optical Continuum and Application to Little Red Dots

  • Authors: Yi-Xian Chen, Hanpu Liu, Ruancun Li, Bingjie Wang, Yilun Ma, Yan-Fei Jiang, Jenny E. Greene, Eliot Quataert, Jeremy Goodman

Yi-Xian Chen et al 2026 The Astrophysical Journal Letters 1003 .

  • Provider: AAS Journals

Caption: Figure 4.

Radial structure of fiducial disk solutions for M• = 106M⊙, α = 0.1 and outer boundary accretion rates of ﹩\dot{M}=0.1{M}_{\odot }﹩ yr−1, with varying mass-loss slope γ. The midplane temperature T and effective temperature Teff are shown in solid and dashed lines, respectively, in the top left panel. The transition toward an inner viscous α-disk, if present, is indicated by vertical dotted lines.

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