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• W2054901417 abstract "We show that the disruption of a star by a ~106 M☉ black hole in a galactic nucleus could under favorable circumstances produce an optically thick envelope that radiates with a thermal spectrum at the Eddington limit, ~1044 ergs s-1, for tens of years. The low apparent temperature of this envelope, ~104 K, would be easily detectable in optical surveys. If most galaxies harbor a massive black hole at their center, then the Sloan Digital Sky Survey might find hundreds of galaxies with nuclear activity of this type. Because the envelope is driven to shine near the Eddington limit, a measurement of the source redshift and total luminosity could yield the black hole mass." @default.
• W2054901417 created "2016-06-24" @default.
• W2054901417 creator A5014157743 @default.
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• W2054901417 date "1997-11-10" @default.
• W2054901417 modified "2023-10-09" @default.
• W2054901417 title "Optical Appearance of the Debris of a Star Disrupted by a Massive Black Hole" @default.
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• W2054901417 doi "https://doi.org/10.1086/304814" @default.
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