Bolometric Corrections for FU Ori Object Accretion Disk Luminosities

The accretion luminosity of an FU Ori disk is a fundamental system parameter, but a challenging one to estimate for all but the most well-studied systems. FU Ori objects are dynamically evolving accretion disks, especially close in time to the outburst epoch. They have a complex multitemperature dis...

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Bibliographic Details
Main Authors: Adolfo S. Carvalho, Lynne A. Hillenbrand
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal Letters
Subjects:
Online Access:https://doi.org/10.3847/2041-8213/ad8cdf