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Tidal Disruptions of Main Sequence Stars - II. Simulation Methodology and Stellar Mass Dependence of the Character of Full Tidal Disruptions

The Astrophysical journal, 2020-12, Vol.904 (98) [Peer Reviewed Journal]

Copyright Determination: MAY_INCLUDE_COPYRIGHT_MATERIAL ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/abb3cf

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  • Title:
    Tidal Disruptions of Main Sequence Stars - II. Simulation Methodology and Stellar Mass Dependence of the Character of Full Tidal Disruptions
  • Author: Ryu, Taeho ; Krolik, Julia ; Piran, Tsvi ; Noble, Scott Charles
  • Subjects: Astronomy
  • Is Part Of: The Astrophysical journal, 2020-12, Vol.904 (98)
  • Description: This paper introduces a series of papers presenting a quantitative theory for the tidal disruption of main-sequence stars by supermassive black holes. Using fully general relativistic hydrodynamics simulations and MESA-model initial conditions, we explore the pericenter-dependence of tidal disruption properties for eight stellar masses (0.15 < M_/M<10)and six black hole masses( ́10
  • Publisher: Goddard Space Flight Center: American Astronomical Society, IOP
  • Language: English
  • Identifier: ISSN: 0004-637X
    EISSN: 1538-4357
    DOI: 10.3847/1538-4357/abb3cf
  • Source: NASA Technical Reports Server
    Alma/SFX Local Collection
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