H I versus H α – comparing the kinematic tracers in modelling the initial conditions of the Mice-Reference-Cited by-同舟云学术

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H I versus H α – comparing the kinematic tracers in modelling the initial conditions of the Mice

Published:2017-11-20 Issue:3 Volume:474 Page:3423-3434
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Mortazavi S Alireza^ORCID,Lotz Jennifer M,Barnes Joshua E,Privon George C^ORCID,Snyder Gregory F

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/474/3/3423/23002090/stx2964.pdf

Reference51 articles.

1. Shock-induced star formation in a model of the Mice

2. Identikit 2: an algorithm for reconstructing galactic collisions

3. Transformations of galaxies – III. Encounter dynamics and tidal response as functions of galaxy structure

Cited by 2 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Dynamics and shocks from H α emission of nearby galaxy mergers;Monthly Notices of the Royal Astronomical Society;2019-05-29

2. Quenching or Bursting: The Role of Stellar Mass, Environment, and Specific Star Formation Rate to $z\sim 1$;The Astrophysical Journal;2018-02-01

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