J
Julio F. Navarro
Researcher at University of Victoria
Publications - 393
Citations - 79749
Julio F. Navarro is an academic researcher from University of Victoria. The author has contributed to research in topics: Galaxy & Dark matter. The author has an hindex of 113, co-authored 376 publications receiving 72998 citations. Previous affiliations of Julio F. Navarro include University of Massachusetts Amherst & Alfred P. Sloan Foundation.
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Journal ArticleDOI
The many lives of active galactic nuclei: cooling flows, black holes and the luminosities and colours of galaxies
Darren J. Croton,Volker Springel,Simon D. M. White,G. De Lucia,Carlos S. Frenk,Liang Gao,Adrian Jenkins,Guinevere Kauffmann,Julio F. Navarro,Naoki Yoshida +9 more
TL;DR: In this article, the authors simulate the growth of galaxies and their central supermassive black holes by implementing a suite of semi-analytic models on the output of the Millennium Run, a very large simulation of the concordance LCDM cosmogony.
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Constraining the Galaxy's dark halo with RAVE stars
T. Piffl,James Binney,Paul J. McMillan,Matthias Steinmetz,Amina Helmi,Rosemary F. G. Wyse,Olivier Bienaymé,Joss Bland-Hawthorn,Kenneth C. Freeman,Brad K. Gibson,Brad K. Gibson,Gerard Gilmore,Eva K. Grebel,Georges Kordopatis,Julio F. Navarro,Quentin A. Parker,Quentin A. Parker,Warren A. Reid,George M. Seabroke,Arnaud Siebert,Fred G. Watson,Tomaž Zwitter +21 more
TL;DR: In this paper, the authors used the kinematics of ∼200000 giant stars that lie within 1.5kpc of the plane to measure the vertical profile of mass density near the Sun.
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Galaxy-Induced Transformation of Dark Matter Halos
TL;DR: In this article, the shape of the halo becomes more axisymmetric: halos are transformed from triaxial into essentially oblate systems, with well-aligned isopotential contours of roughly constant flattening (c/a ~ 0.85).
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The Phoenix Project: the dark side of rich galaxy clusters
Liang Gao,Julio F. Navarro,Carlos S. Frenk,Adrian Jenkins,Volker Springel,Volker Springel,Stephen White +6 more
TL;DR: The Phoenix Project as discussed by the authors is a set of Λ cold dark matter (CDM) simulations of the dark matter component of nine rich galaxy clusters, each cluster is simulated at least at two different numerical resolutions.
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The cosmological origin of the Tully-Fisher relation
TL;DR: In this paper, the authors use high-resolution cosmological simulations that include the effects of gasdynamics and star formation to investigate the origin of the Tully-Fisher relation in the standard Cold Dark Matter cosmogony.