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Tidal Disruptions of Main Sequence Stars - II. Simulation Methodology and Stellar Mass Dependence of the Character of Full Tidal DisruptionsThis 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
Document ID
20205011634
Acquisition Source
Goddard Space Flight Center
Document Type
Reprint (Version printed in journal)
Authors
Taeho Ryu (Johns Hopkins University Baltimore, Maryland, United States)
Julia Krolik (Johns Hopkins University Baltimore, Maryland, United States)
Tsvi Piran (Hebrew University of Jerusalem Jerusalem, Israel)
Scott Charles Noble (Goddard Space Flight Center Greenbelt, Maryland, United States)
Date Acquired
December 16, 2020
Publication Date
December 1, 2020
Publication Information
Publication: The Astrophysical Journal
Publisher: American Astronomical Society, IOP
Volume: 904
Issue: 98
Issue Publication Date: December 1, 2020
ISSN: 0004-637X
e-ISSN: 1538-4357
DOI: doi: 10.3847/1538-4357/abb3cf
Subject Category
Astronomy
Funding Number(s)
WBS: 244904.04.09.05.04.03
Distribution Limits
Public
Copyright
Portions of document may include copyright protected material.
Technical Review
External Peer Committee
Document Inquiry

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