S
Sijing Shen
Researcher at University of California, Santa Cruz
Publications - 62
Citations - 6707
Sijing Shen is an academic researcher from University of California, Santa Cruz. The author has contributed to research in topics: Galaxy & Star formation. The author has an hindex of 38, co-authored 59 publications receiving 6330 citations. Previous affiliations of Sijing Shen include University of Cambridge & McMaster University.
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Cuspy no more: How outflows affect the central dark matter and baryon distribution in Λ cold dark matter galaxies
Fabio Governato,Adi Zolotov,Andrew Pontzen,Charlotte Christensen,Se-Heon Oh,Se-Heon Oh,Alyson Brooks,Thomas R. Quinn,Sijing Shen,James Wadsley +9 more
TL;DR: In this article, the authors examined the evolution of the inner dark matter (DM) and baryonic density profile of simulated field galaxies using fully cosmological, CDM, high resolution SPH + N-Body simulations.
Journal ArticleDOI
Cuspy No More: How Outflows Affect the Central Dark Matter and Baryon Distribution in Lambda CDM Galaxies
Fabio Governato,Adi Zolotov,Andrew Pontzen,Charlotte Christensen,Se-Heon Oh,Alyson Brooks,Thomas R. Quinn,Sijing Shen,James Wadsley +8 more
TL;DR: In this paper, the authors examined the evolution of the inner dark matter (DM) and baryonic density profile of simulated field galaxies using fully cosmological, Lambda CDM, high resolution SPH + N-Body simulations.
Journal ArticleDOI
The enrichment of the intergalactic medium with adiabatic feedback - I. Metal cooling and metal diffusion
TL;DR: In this paper, a study of metal enrichment of the intergalactic medium (IGM) using a series of smooth particle hydrodynamics (SPH) simulations is presented, employing models for metal cooling and the turbulent diffusion of metals and thermal energy.
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Baryons matter: why luminous satellite galaxies have reduced central masses
Adi Zolotov,Alyson Brooks,Beth Willman,Fabio Governato,Andrew Pontzen,Charlotte Christensen,Avishai Dekel,Thomas P. Quinn,Sijing Shen,James Wadsley +9 more
TL;DR: In this article, high-resolution cosmological hydrodynamical simulations of Milky Way-massed disk galaxies are used to demonstrate that supernovae feedback and tidal stripping lower the central masses of bright (15 < MV < 8) satellite galaxies.
Journal ArticleDOI
The AGORA high-resolution galaxy simulations comparison project
Ji-hoon Kim,Tom Abel,Oscar Agertz,Oscar Agertz,Greg L. Bryan,Daniel Ceverino,Charlotte Christensen,Charlie Conroy,Avishai Dekel,Nickolay Y. Gnedin,Nickolay Y. Gnedin,Nathan J. Goldbaum,Javiera Guedes,Oliver Hahn,Alexander Hobbs,Philip F. Hopkins,Philip F. Hopkins,Cameron Hummels,Francesca Iannuzzi,Dušan Kereš,Anatoly Klypin,Andrey V. Kravtsov,Mark R. Krumholz,Michael Kuhlen,Michael Kuhlen,Samuel N. Leitner,Piero Madau,Lucio Mayer,Christopher E. Moody,Kentaro Nagamine,Kentaro Nagamine,Michael L. Norman,Jose Oñorbe,Brian W. O'Shea,Annalisa Pillepich,Joel R. Primack,Thomas R. Quinn,Justin I. Read,Brant Robertson,Miguel Rocha,Douglas H. Rudd,Sijing Shen,Britton D. Smith,Alexander S. Szalay,Romain Teyssier,Robert Thompson,Robert Thompson,Keita Todoroki,Matthew J. Turk,James Wadsley,John H. Wise,and Adi Zolotov +51 more
TL;DR: AGORA as mentioned in this paper is a comprehensive numerical study of well-resolved galaxies within the ΛCDM cosmology, which is run with a variety of code platforms to follow the hierarchical growth, star formation history, morphological transformation, and the cycle of baryons in and out of eight galaxies with halo masses M = 0.