activity
19972005
most citedMinihalo photoevaporation during cosmic reionization: evaporation times and photon consumption rates

154 citations · 166 across the 6 of their papers we have counts for

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13 papers · 1 filter

astro-ph20052 cited

Ionization fronts and their interaction with density fluctuations: implications for reionization

Ilian T. Iliev, Paul R. Shapiro, Evan Scannapieco +4

The propagation of cosmological ionization fronts (I-fronts) during reionization is strongly influenced by small-scale structure. Here we summarize our recent attemps to understand…

astro-ph20052 cited

The interaction of a jet-like pulse with a wind from a stellar companion

A. Riera, A. C. Raga, J. Alcolea

We present numerical simulations of the interaction between a collimated, bipolar ``pulse'' ejected from a star and a continuous wind ejected from a stellar companion. We explore t…

astro-ph2004154 cited

Minihalo photoevaporation during cosmic reionization: evaporation times and photon consumption rates

Ilian T. Iliev, Paul R. Shapiro, Alejandro C. Raga

The weak, R-type ionization fronts (I-fronts) which swept across the intergalactic medium (IGM) during the reionization of the universe often found their paths blocked by cosmologi…

astro-ph20043 cited

Hydrodynamical interaction between an accretion flow and a stellar wind

S. Mendoza, J. Canto, A. Raga

Molecular clouds in the interstellar medium suffer gravitational instabilities that lead to the formation of one or multiple stars. A recently formed star inside a cold cloud commu…

astro-ph20033 cited

A model for the cross section of a turbulent, radiative jet or wake

J. Canto, A. C. Raga, A. Riera

We present an analytical model for the cross section of a turbulent, radiative jet or wake. This model is appropriate for modeling HH jets, or "wakes" left behind by "astrophysical…

astro-ph20032 cited

Relation between source and temperature fluctuations in photoionized nebulae

Luc Binette, Pierre Ferruit, Wolfgang Steffen +1

The magnitude of the temperature fluctuations (t^2) required to explain the observed inconsistencies between metallicities inferred from recombination lines and from forbidden line…