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BUDHIES II: A phase-space view of HI gas stripping and star-formation quenching in cluster galaxies

Y. Jaffe, R. Smith, G. Candlish, B. Poggianti, Y. Sheen, и M. Verheijen. (2015)cite arxiv:1501.03819Comment: Accepted for publication by MNRAS; 16 pages and 10 Figures (including Appendix).

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Rory Tews

Rory Christopher Holmes

David Smith

Stephen Smith

Veronica Smith

Другие публикации лиц с тем же именем

A History of HI Stripping in Virgo: A Phase-space View of VIVA GalaxiesH. Yoon, A. Chung, R. Smith, и Y. Jaffé. (2017)cite arxiv:1704.00760Comment: 16 pages, 8 figures, 1 table, accepted for publication in ApJ.MUSE-ings on AM1354-250: Collisions, Shocks and RingsB. Conn, L. Fogarty, R. Smith, и G. Candlish. (2015)cite arxiv:1512.07667Comment: 10 pages, 10 figures, ESO/MUSE Science Verification data, Final DataCube will be provided on request. Accepted for publication in ApJ.DeepKey: Towards End-to-End Physical Key Replication from a Single Photograph.R. Smith, и T. Burghardt. GCPR, том 11269 из Lecture Notes in Computer Science, стр. 487-502. Springer, (2018)BUDHIES III: The fate of HI and the quenching of galaxies in evolving environmentsY. Jaffé, M. Verheijen, C. Haines, H. Yoon, R. Cybulski, M. Montero-Castaño, R. Smith, A. Chung, B. Deshev, X. Fernández и 6 other автор(ы). (2016)cite arxiv:1604.07832Comment: 21 pages (including appendix). Accepted for publication in MNRAS.Discovery of ram pressure stripped gas around an elliptical galaxy in Abell 2670Y. Sheen, R. Smith, Y. Jaffe, M. Kim, S. Yi, P. Duc, J. Nantais, G. Candlish, R. Demarco, и E. Treister. (2017)cite arxiv:1704.05173Comment: 6 pages, 5 figures, accepted for publication in ApJL.Phase-space Analysis in the Group and Cluster environment: Time since Infall and Tidal Mass LossJ. Rhee, R. Smith, H. Choi, S. Yi, Y. Jaffé, G. Candlish, и R. Sanchez-Janssen. (2017)cite arxiv:1704.04243Comment: Accepted to ApJ 13 April 2017, 14 pages, 9 figures.BUDHIES II: A phase-space view of HI gas stripping and star-formation quenching in cluster galaxiesY. Jaffe, R. Smith, G. Candlish, B. Poggianti, Y. Sheen, и M. Verheijen. (2015)cite arxiv:1501.03819Comment: Accepted for publication by MNRAS; 16 pages and 10 Figures (including Appendix).

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