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Title: ON THE ROLE OF DISKS IN THE FORMATION OF STELLAR SYSTEMS: A NUMERICAL PARAMETER STUDY OF RAPID ACCRETION

Journal Article · · Astrophysical Journal
;  [1];  [2];  [3]
  1. Department of Astronomy and Astrophysics, 50 St. George Street, University of Toronto, Toronto, Ontario M5R 3H4 (Canada)
  2. Department of Astronomy, 201 Interdisciplinary Sciences Building, University of California, Santa Cruz, CA 95064 (United States)
  3. Department of Astronomy, University of California, Berkeley 601 Campbell Hall, Berkeley, CA 94720-3411 (United States)

We study rapidly accreting, gravitationally unstable disks with a series of idealized global, numerical experiments using the code ORION. Our numerical parameter study focuses on protostellar disks, showing that one can predict disk behavior and the multiplicity of the accreting star system as a function of two dimensionless parameters which compare the infall rate to the disk sound speed and orbital period. Although gravitational instabilities become strong, we find that fragmentation into binary or multiple systems occurs only when material falls in several times more rapidly than the canonical isothermal limit. The disk-to-star accretion rate is proportional to the infall rate and governed by gravitational torques generated by low-m spiral modes. We also confirm the existence of a maximum stable disk mass: disks that exceed approx50% of the total system mass are subject to fragmentation and the subsequent formation of binary companions.

OSTI ID:
21392393
Journal Information:
Astrophysical Journal, Vol. 708, Issue 2; Other Information: DOI: 10.1088/0004-637X/708/2/1585; ISSN 0004-637X
Country of Publication:
United States
Language:
English

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Decoupling of Magnetic Fields in Collapsing Protostellar Envelopes and Disk Formation and Fragmentation text January 2017
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