activity
20032025
most citedWinds from clu\sters with non-uniform stellar distributions

25 citations · 91 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.SR2025

HH 270/110 as a jet/shear layer interaction

A. C. Raga, A. Noriega-Crespo, A. Castellanos-Ramirez +5

New observations obtained with JWST of the proto-stellar HH~270 jet and the "deflected" HH 110 system, show that HH 110 has a morphology of a series of distorted working surfaces.…

astro-ph.SR2020★ 2 cited

A "head/tail" plasmon model with a Hubble law velocity profile

A. C. Raga, A. Rodriguez-Gonzalez, L. Hernande-Martinez +2

We present a model of a hypersonic, collimated, "single pulse" outflow, produced by an event with an ejection velocity that first grows, reaches a peak, and then decreases again to…

astro-ph.GA2012★ 15 cited

Gravitational drag on a point mass in hypersonic motion within a Gaussian disk

J. Cantó, A. Esquivel. F. J. Sánchez-Salcedo, A. C. Raga

We develop an analytical model for the accretion and gravitational drag on a point mass that moves hypersonically in the midplane of a gaseous disk with a Gaussian vertical density…

astro-ph.GA2011★ 18 cited

Gravitational drag on a point mass in hypersonic motion through a gaseous medium

J. Canto, A. C. Raga, A. Esquivel +1

We explore a ballistic orbit model to infer the gravitational drag force on an accreting point mass M, such as a black hole, moving at a hypersonic velocity v_{0} through a gaseous…

astro-ph.HE2011

The cometary cavity created by an aligned streaming environment/collimated outflow interaction

D. López-Cámara, A. Esquivel, J. Cantó +3

We present a "thin shell" model of the interaction of a biconical outflow and a streaming environment (aligned with the direction of the flow), as well as numerical (axisymmetric)…

astro-ph.GA2010★ 24 cited

A model of Mira's cometary head/tail entering the Local Bubble

A. Esquivel, A. C. Raga, J. Canto +4

We model the cometary structure around Mira as the interaction of an AGB wind from Mira A, and a streaming environment. Our simulations introduce the following new element: we assu…