Zobrazeno 1 - 6
of 6
pro vyhledávání: '"Arraki, Kenza S."'
Autor:
Kim, Ji-hoon, Agertz, Oscar, Teyssier, Romain, Butler, Michael J., Ceverino, Daniel, Choi, Jun-Hwan, Feldmann, Robert, Keller, Ben W., Lupi, Alessandro, Quinn, Thomas, Revaz, Yves, Wallace, Spencer, Gnedin, Nickolay Y., Leitner, Samuel N., Shen, Sijing, Smith, Britton D., Thompson, Robert, Turk, Matthew J., Abel, Tom, Arraki, Kenza S., Benincasa, Samantha M., Chakrabarti, Sukanya, DeGraf, Colin, Dekel, Avishai, Goldbaum, Nathan J., Hopkins, Philip F., Hummels, Cameron B., Klypin, Anatoly, Li, Hui, Madau, Piero, Mandelker, Nir, Mayer, Lucio, Nagamine, Kentaro, Nickerson, Sarah, O'Shea, Brian W., Primack, Joel R., Roca-Fàbrega, Santi, Semenov, Vadim, Shimizu, Ikkoh, Simpson, Christine M., Todoroki, Keita, Wadsley, James W., Wise, John H.
Publikováno v:
Astrophysical Journal, 833, 202, 2016
Using an isolated Milky Way-mass galaxy simulation, we compare results from 9 state-of-the-art gravito-hydrodynamics codes widely used in the numerical community. We utilize the infrastructure we have built for the AGORA High-resolution Galaxy Simula
Externí odkaz:
http://arxiv.org/abs/1610.03066
Dwarf spheroidal galaxies (dSphs) are extremely gas-poor, dark matter-dominated galaxies, which make them ideal to test the predictions of the cold dark matter (CDM) model. We argue that the removal of the baryonic component from gas-rich dwarf irreg
Externí odkaz:
http://arxiv.org/abs/1212.6651
Broad absorption line (BAL) quasars probe the high velocity gas ejected by luminous accreting black holes. BAL variability timescales place constraints on the size, location, and dynamics of the emitting and absorbing gas near the supermassive black
Externí odkaz:
http://arxiv.org/abs/1201.2895
Akademický článek
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Akademický článek
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K zobrazení výsledku je třeba se přihlásit.
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Autor:
Kim, Ji-Hoon, Agertz, Oscar, Teyssier, Romain, Butler, Michael J., Ceverino, Daniel, Choi, Jun-Hwan, Feldmann, Robert, Keller, Ben W., Lupi, Alessandro, Quinn, Thomas, Revaz, Yves, Wallace, Spencer, Gnedin, Nickolay Y., Leitner, Samuel N., Shen, Sijing, Smith, Britton D., Thompson, Robert, Turk, Matthew J., Abel, Tom, Arraki, Kenza S., Benincasa, Samantha M., Chakrabarti, Sukanya, Degraf, Colin, Dekel, Avishai, Goldbaum, Nathan J., Hopkins, Philip F., Hummels, Cameron B., Klypin, Anatoly, Hui Li, Madau, Piero, Mandelker, Nir, Mayer, Lucio, Nagamine, Kentaro, Nickerson, Sarah, O Shea, Brian W., Primack, Joel R., Roca-Fàbrega, Santi, Semenov, Vadim, Shimizu, Ikkoh, Simpson, Christine M., Todoroki, Keita, Wadsley, James W., Wise, John H., Agora, For The Collaboration
Publikováno v:
NASA Astrophysics Data System
Using an isolated Milky Way-mass galaxy simulation, we compare results from nine state-of-the-art gravitohydrodynamics codes widely used in the numerical community. We utilize the infrastructure we have built for the AGORA High-resolution Galaxy Simu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::22c75ddb06a933d73a128e4fc40bbeeb
https://ui.adsabs.harvard.edu/#abs/2016arXiv161003066K
https://ui.adsabs.harvard.edu/#abs/2016arXiv161003066K