activity
20022009
most citedMultiple and Precessing Collimated Outflows in the Planetary Nebula IC 4634

43 citations · 77 across the 4 of their papers we have counts for

collaborators
Showing astro-phShow all

6 papers · 1 filter

astro-ph200843 cited

Multiple and Precessing Collimated Outflows in the Planetary Nebula IC 4634

M. A. Guerrero, L. F. Miranda, A. Riera +6

With its remarkable double-S shape, IC 4634 is an archetype of point-symmetric planetary nebulae (PN). In this paper, we present a detailed study of this PN using archival HST WFPC…

astro-ph200721 cited

A precessing jet model for the PN K 3-35: simulated radio-continuum emission

P. Velazquez, Y. Gomez, A. Esquivel +1

The bipolar morphology of the planetary nebula (PN) K 3-35 observed in radio-continuum images was modelled with 3D hydrodynamic simulations with the adaptive grid code yguazu-a. We…

astro-ph2005

Emission lines from rotating proto-stellar jets with variable velocity profiles. I. Three-dimensional numerical simulation of the non-magnetic case

A. H. Cerqueira, P. F. Velazquez, A. C. Raga +2

Using the Yguazu-a three-dimensional hydrodynamic code, we have computed a set of numerical simulations of heavy, supersonic, radiatively cooling jets including variabilities in bo…

astro-ph2004

Numerical Modeling of Eta Carinae Bipolar Outflows

R. F. Gonzalez, E. M. de Gouveia Dal Pino, A. C. Raga +1

In this paper, we present two-dimensional gas dynamic simulations of the formation and evolution of the eta-Car bipolar outflows. Adopting the interacting nonspherical winds model,…

astro-ph2004

Time-dependent ejection velocity model for the outflow of Hen 3--1475

P. F. Velazquez, A. Riera, A. C. Raga

We present 2D axisymmetric and 3D numerical simulations of the proto-planetary nebula Hen 3-1475, which is characterized by a remarkably highly collimated optical jet, formed by a…

astro-ph2002

A Supernova Remnant Collision with a Stellar Wind

Pablo F. Velazquez, Gloria Koenigsberger, Alejandro C. Raga

Numerical simulations of the interaction between supernova ejecta and a stellar wind are presented. We follow the temporal evolution of the shock fronts that are formed through suc…