A systematic analysis of star cluster disruption by tidal shocks – I. Controlled N-body simulations and a new theoretical model-Reference-Cited by-同舟云学术

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A systematic analysis of star cluster disruption by tidal shocks – I. Controlled N-body simulations and a new theoretical model

Published:2019-05-08 Issue:4 Volume:486 Page:5879-5894
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Webb Jeremy J¹,Reina-Campos Marta²^ORCID,Kruijssen J M Diederik²^ORCID

Affiliation:

1. Department of Astronomy and Astrophysics, University of Toronto, 50 St George Street, Toronto, ON M5S 3H4, Canada

2. Astronomisches Rechen-Institut, Zentrum für Astronomie der Universität Heidelberg, Mönchhofstraße 12-14, D-69120 Heidelberg, Germany

Funder

Natural Sciences and Engineering Research Council of Canada

European Research Council

California Department of Fish and Game

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/advance-article-pdf/doi/10.1093/mnras/stz1264/28571239/stz1264.pdf

Reference65 articles.

1. Gravitational N-Body Simulations

2. On the evolution of globular cluster systems. I - Present characteristics and rate of destruction in our Galaxy

3. Tidal interactions between spherical galaxies

4. The density profiles of tidally stripped galaxies

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