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pro vyhledávání: '"Brown, Gillen"'
Autor:
Brown, Gillen, Gnedin, Oleg Y.
We present a suite of galaxy formation simulations that directly model star cluster formation and disruption. Starting from a model previously developed by our group, here we introduce several improvements to the prescriptions for cluster formation a
Externí odkaz:
http://arxiv.org/abs/2203.00559
Autor:
Brown, Gillen, Gnedin, Oleg Y.
We measure the projected half-light radii of young star clusters in 31 galaxies from the Legacy Extragalactic UV Survey (LEGUS). We implement a custom pipeline specifically designed to be robust against contamination, which allows us to measure radii
Externí odkaz:
http://arxiv.org/abs/2106.12420
Autor:
Brown, Gillen, Gnedin, Oleg Y.
We present a method for customizing the root grid of zoom-in initial conditions used for simulations of galaxy formation. Starting from the white noise used to seed the structures of an existing initial condition, we cut out a smaller region of inter
Externí odkaz:
http://arxiv.org/abs/2009.09085
Autor:
Gonzalez, Anthony H., Gettings, Daniel P., Brodwin, Mark, Eisenhardt, Peter R. M., Stanford, S. Adam, Wylezalek, Dominika, Decker, Bandon, Marrone, Daniel P., Moravec, Emily, O'Donnell, Christine, Stalder, Brian, Stern, Daniel, Abdulla, Zubair, Brown, Gillen, Carlstrom, John, Chambers, Kenneth C., Hayden, Brian, Lin, Yen-Ting, Magnier, Eugene, Masci, Frank, Mantz, Adam B., McDonald, Michael, Mo, Wenli, Perlmutter, Saul, Wright, Edward L., Zeimann, Gregory R.
We present the Massive and Distant Clusters of WISE Survey (MaDCoWS), a search for galaxy clusters at 0.7
Externí odkaz:
http://arxiv.org/abs/1809.06820
Publikováno v:
Brown et. al. 2018, ApJ, 864, 94
We investigate the possible connection between the most massive globular clusters, such as $\omega$ Cen and M54, and nuclear star clusters of dwarf galaxies that exhibit similar spreads in age and metallicity. We examine galactic nuclei in cosmologic
Externí odkaz:
http://arxiv.org/abs/1804.09819
Autor:
Brown, Gillen
I present my work to measure the radii of observed star clusters and investigate the formation and evolution of star clusters with cosmological simulations. By measuring the radii of over 6000 young star clusters in 31 nearby galaxies, I find that ga
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::13aef18a079a27e100fdcde967869cc6
Akademický článek
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Autor:
Gordon L. Patzer
Physical attractiveness phenomena permeate society with somber ramifica tions. Correspondingly, practical applications of physical attractiveness phenomena are extensive. The consequence is that almost every person can benefit from knowledge about