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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Dynamical effects of dark matter in systems of galaxies
TL;DR: In this article, mass estimates from the dynamics of the luminous component (MVT) under the influence of such a background, assuming a constant dark/luminous mass ratio and plausible physical conditions, were discussed.
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Dark Matter Halos and Disk Rotation Curves
TL;DR: In this article, it was shown that the spherically averaged density profiles of dark matter halos have a universal shape and the logarithmic slope of this profile is shallower than isothermal near the center, and steepens gently outwards, becoming steeper than the halo virial radius.
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Distance determination for RAVE stars using stellar models
Maarten A. Breddels,M. C. Smith,Amina Helmi,Olivier Bienaymé,James Binney,Joss Bland-Hawthorn,Corrado Boeche,Benedict C M Burnett,Randy D. Campbell,Kenneth C. Freeman,Brad K. Gibson,Gerard Gilmore,Eva K. Grebel,Ulisse Munari,Julio F. Navarro,Quentin A. Parker,George M. Seabroke,Arnaud Siebert,Alessandro Siviero,Matthias Steinmetz,Fred G. Watson,Mary E K Williams,Rosemary F. G. Wyse,Tomaž Zwitter +23 more
TL;DR: In this article, the authors used stellar models combined with atmospheric properties from RAVE (Teff, logg and [Fe/H]) and (J-Ks) photometry from archival sources to derive absolute magnitudes.
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Disk galaxies at z=2 in OWLS
TL;DR: In this paper, the effect of supernova feedback from evolving stars on the baryonic mass and angular momentum content of galaxies that assemble at the center of 1e11-3e12 h^{-1}M_\odot halos was studied.
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The Tucana dwarf spheroidal: a distant backsplash galaxy of M31?
TL;DR: Tucana dSph, one of the few known quiescent LG field dwarfs, at dM31 ≈ 1350kpc and dMW ≈ 880kpc, is a promising candidate as mentioned in this paper .