Sijing Shen
University of Cambridge
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Publication
Featured researches published by Sijing Shen.
The Astrophysical Journal | 2015
Sijing Shen; Ryan J. Cooke; Enrico Ramirez-Ruiz; Piero Madau; Lucio Mayer; Javiera Guedes
We investigate the production sites and the enrichment history of
The Astrophysical Journal | 2015
Lucio Mayer; Davide Fiacconi; Silvia Bonoli; Thomas P. Quinn; Rok Roskar; Sijing Shen; James Wadsley
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Monthly Notices of the Royal Astronomical Society | 2015
Valentina Tamburello; Lucio Mayer; Sijing Shen; James Wadsley
-process elements in the Galaxy, as traced by the [Eu/Fe] ratio, using the high resolution, cosmological zoom-in simulation `Eris. At
The Astrophysical Journal | 2016
Jihoon Kim; Oscar Agertz; Romain Teyssier; Michael J. Butler; Daniel Ceverino; Jun-Hwan Choi; Robert Feldmann; Ben W. Keller; Alessandro Lupi; Thomas P. Quinn; Y. Revaz; Spencer Wallace; Nickolay Y. Gnedin; Samuel N. Leitner; Sijing Shen; Britton D. Smith; Robert Thompson; Matthew J. Turk; Tom Abel; Kenza S. Arraki; Samantha M. Benincasa; Sukanya Chakrabarti; Colin DeGraf; Avishai Dekel; Nathan J. Goldbaum; Philip F. Hopkins; Cameron B. Hummels; Anatoly Klypin; Hui Li; Piero Madau
z=0
The Astrophysical Journal | 2016
Aleksandra Sokołowska; Lucio Mayer; Arif Babul; Piero Madau; Sijing Shen
, Eris represents a close analog to the Milky Way, making it the ideal laboratory to understand the chemical evolution of our Galaxy. Eris formally traces the production of oxygen and iron due to Type-Ia and Type-II supernovae. We include in post-processing the production of
Monthly Notices of the Royal Astronomical Society | 2017
R. O'Shaughnessy; Jillian M. Bellovary; Alyson M. Brooks; Sijing Shen; Fabio Governato; Charlotte R. Christensen
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The Astrophysical Journal | 2017
Aleksandra Sokołowska; Pedro R. Capelo; S. Michael Fall; Lucio Mayer; Sijing Shen; Silvia Bonoli
-process elements from compact binary mergers. Unlike previous studies, we find that the nucleosynthetic products from compact binary mergers can be incorporated into stars of very low metallicity and at early times, even with a minimum delay time of 100 Myr. This conclusion is relatively insensitive to modest variations in the merger rate, minimum delay time, and the delay time distribution. By implementing a first-order prescription for metal-mixing, we can further improve the agreement between our model and the data for the chemical evolution of both [
The Astrophysical Journal | 2016
Gabriela Montes; Enrico Ramirez-Ruiz; Jill Naiman; Sijing Shen; William H. Lee
alpha
Monthly Notices of the Royal Astronomical Society | 2017
Sijing Shen; Girish Kulkarni; Piero Madau; Lucio Mayer
/Fe] and [Eu/Fe].We argue that compact binary mergers could be the dominant source of
The Astrophysical Journal | 2017
Andrew A. Cole; Daniel R. Weisz; Evan D. Skillman; Ryan Leaman; Benjamin F. Williams; Andrew E. Dolphin; L. Clifton Johnson; Alan W. McConnachie; Michael Boylan-Kolchin; Julianne J. Dalcanton; Fabio Governato; Piero Madau; Sijing Shen; Mark Vogelsberger
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