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20032026
most citedSubhaloes in Self-Interacting Galactic Dark Matter Haloes

570 citations · 5.4k across the 78 of their papers we have counts for

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8 papers · 1 filter

astro-ph2008★ 86 cited

On the baryonic, stellar, and luminous scaling relations of disk galaxies

V. Avila-Reese, J. Zavala, C. Firmani +1

We explore how the slopes and scatters of the scaling relations of disk galaxies (Vm-L[-M], R-L[-M], and Vm-R) do change when moving from B to K bands and to stellar and baryonic q…

astro-ph2008★ 1 cited

Constraining the mSUGRA parameter space using the entropy of dark matter halos

Dario Nunez, Jesus Zavala, Lukas Nellen +3

We derive an expression for the entropy of a dark matter halo described by a Navarro-Frenk-White model with a core. The comparison of this entropy with the one of dark matter at th…

astro-ph2008★ 2 cited

3D hydrodynamical simulations of the large scale structure of W50-SS433

Jesús Zavala, Pablo F. Velázquez, Adriano H. Cerqueira +1

We present 3D hydrodynamical simulations of a precessing jet propagating inside a supernova remnant (SNR) shell, particularly applied to the W50-SS433 system in a search for the or…

astro-ph2006★ 28 cited

Stellar polytropes and Navarro-Frenk-White halo models: comparison with observations

Jesus Zavala, Dario Nunez, Roberto A. Sussman +2

Motivated by the possible conflict between the Navarro-Frenk-White(NFW) model predictions for the dark matter contents of galactic systems and its correlation with baryonic surface…

astro-ph2006★ 1 cited

Entropy considerations in constraining the mSUGRA parameter space

Dario Nunez, Roberto A. Sussman, Jesus Zavala +3

We explore the use of two criteria to constraint the allowed parameter space in mSUGRA models. Both criteria are based in the calculation of the present density of neutralinos as d…

astro-ph2005★ 10 cited

Pioneer anomaly? Gravitational pull due to the Kuiper belt

Jose A. de Diego, Dario Nunez, Jesus Zavala

In this work we study the gravitational influence of the material extending from Uranus orbit to the Kuiper belt and beyond on objects moving within these regions. We conclude that…