Daniel Ceverino
Heidelberg University
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Publication
Featured researches published by Daniel Ceverino.
Monthly Notices of the Royal Astronomical Society | 2014
Daniel Ceverino; Anatoly Klypin; Elizabeth S. Klimek; Sebastian Trujillo-Gomez; Christopher W. Churchill; Joel R. Primack; Avishai Dekel
Any successful model of galaxy formation needs to explain the low rate of star formation in the small progenitors of todays galaxies. This inefficiency is necessary for reproducing the low stellar-to-virial mass fractions, suggested by current abundance matching models. A possible driver of this low efficiency is the radiation pressure exerted by ionizing photons from massive stars. The effect of radiation pressure in cosmological, zoom-in galaxy formation simulations is modeled as a non-thermal pressure that acts only in dense and optically thick star-forming regions. We also include photoionization and photoheating by massive stars. The full photoionization of hydrogen reduces the radiative cooling in the
The Astrophysical Journal | 2015
Yicheng Guo; Henry C. Ferguson; Eric F. Bell; David C. Koo; Christopher J. Conselice; Mauro Giavalisco; Susan A. Kassin; Yu Lu; Ray A. Lucas; Nir Mandelker; Daniel M. McIntosh; Joel R. Primack; Swara Ravindranath; Guillermo Barro; Daniel Ceverino; Avishai Dekel; Sandra M. Faber; Jerome J. Fang; Anton M. Koekemoer; Kai G. Noeske; Marc Rafelski; Amber N. Straughn
10^{4-4.5}
Monthly Notices of the Royal Astronomical Society | 2014
Nir Mandelker; Avishai Dekel; Daniel Ceverino; Dylan Tweed; Christopher E. Moody; Joel R. Primack
K regime. The main effect of radiation pressure is to regulate and limit the high values of gas density and the amount of gas available for star formation. This maintains a low star formation rate of
Monthly Notices of the Royal Astronomical Society | 2016
Sandro Tacchella; Avishai Dekel; C. Marcella Carollo; Daniel Ceverino; Colin DeGraf; Sharon Lapiner; Nir Mandelker; Joel R. Primack
\sim 1 \ {\rm M_\odot} \ {\rm yr}^{-1}
Monthly Notices of the Royal Astronomical Society | 2015
Sebastian Trujillo-Gomez; Anatoly Klypin; Pedro Colín; Daniel Ceverino; Kenza S. Arraki; Joel R. Primack
in halos with masses about
The Astrophysical Journal | 2014
Guillermo Barro; Jonathan R. Trump; David C. Koo; Avishai Dekel; Susan A. Kassin; Dale D. Kocevski; Sandra M. Faber; Arjen van der Wel; Yicheng Guo; P. G. Pérez-González; Elisa Toloba; Jerome J. Fang; Camilla Pacifici; Raymond C. Simons; Randy Campbell; Daniel Ceverino; Steven L. Finkelstein; Bob Goodrich; Marc Kassis; Anton M. Koekemoer; Nicholas P. Konidaris; Rachael Livermore; James Edward Lyke; Bahram Mobasher; Hooshang Nayyeri; Michael Peth; Joel R. Primack; Luca Rizzi; Rachel S. Somerville; Gregory D. Wirth
10^{11} \ {M_\odot}
The Astrophysical Journal | 2014
A. van der Wel; Yu-Yen Chang; Eric F. Bell; B. Holden; Henry C. Ferguson; Mauro Giavalisco; H.-W. Rix; Rosalind E. Skelton; Katherine E. Whitaker; Ivelina Momcheva; Gabriel B. Brammer; Susan A. Kassin; Marie Martig; Avishai Dekel; Daniel Ceverino; David C. Koo; Mark Mozena; P. G. van Dokkum; Marijn Franx; S. M. Faber; Joel R. Primack
at
Monthly Notices of the Royal Astronomical Society | 2012
Tobias Goerdt; Avishai Dekel; A. Sternberg; Orly Gnat; Daniel Ceverino
z\simeq3
Monthly Notices of the Royal Astronomical Society | 2014
Christopher E. Moody; Yicheng Guo; Nir Mandelker; Daniel Ceverino; Mark Mozena; David C. Koo; Avishai Dekel; Joel R. Primack
. Infrared trapping and photoionization/photoheating processes are secondary effects in this mass range. The galaxies residing in these low-mass halos contain only
Monthly Notices of the Royal Astronomical Society | 2016
Daniel Ceverino; Jorge Sanchez Almeida; Casiana Muñoz Tuñón; Avishai Dekel; Bruce G. Elmegreen; Debra Meloy Elmegreen; Joel R. Primack
\sim0.6\%
