R
Ricardo F. González
Researcher at National Autonomous University of Mexico
Publications - 52
Citations - 2086
Ricardo F. González is an academic researcher from National Autonomous University of Mexico. The author has contributed to research in topics: Stars & Star formation. The author has an hindex of 20, co-authored 51 publications receiving 2001 citations. Previous affiliations of Ricardo F. González include University of São Paulo.
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Molecular Cloud Evolution. II. From Cloud Formation to the Early Stages of Star Formation in Decaying Conditions
Enrique Vázquez-Semadeni,Gilberto C. Gómez,A. Katharina Jappsen,Javier Ballesteros-Paredes,Ricardo F. González,Ralf S. Klessen +5 more
TL;DR: In this article, the formation of giant dense cloud complexes and of stars within them using SPH numerical simulations of the collision of gas streams (inflows) in the WNM at moderately supersonic velocities.
Journal ArticleDOI
Molecular Cloud Evolution II. From cloud formation to the early stages of star formation in decaying conditions
Enrique Vázquez-Semadeni,Gilberto C. Gómez,A. K. Jappsen,Javier Ballesteros-Paredes,Ricardo F. González,Ralf S. Klessen +5 more
TL;DR: In this article, the formation of giant dense cloud complexes and of stars within them was studied by means of SPH numerical simulations of the mildly supersonic collision of gas streams (inflows) in the warm neutral medium (WNM).
Journal ArticleDOI
Molecular cloud evolution. i. molecular cloud and thin cold neutral medium sheet formation
TL;DR: In this paper, the authors discuss molecular cloud formation by large-scale supersonic compressions in the diffuse warm neutral medium (WNM) and show that a shocked layer forms, and within it, a thin cold layer.
Journal ArticleDOI
Molecular cloud evolution. I. Molecular cloud and thin CNM sheet formation
TL;DR: In this paper, the authors discuss molecular cloud formation by large-scale supersonic compressions in the diffuse warm neutral medium (WNM) and show that a shocked layer forms, and within it, a thin cold layer.
Journal ArticleDOI
The nature of the velocity field in molecular clouds - I. The non-magnetic case
Enrique Vázquez-Semadeni,Ricardo F. González,Javier Ballesteros-Paredes,Adriana Gazol,Jongsoo Kim +4 more
TL;DR: In this article, a set of three numerical simulations of randomly driven, isothermal, non-magnetic, self-gravitating turbulence with different rms Mach numbers and physical sizes, but with approximately the same value of the virial parameter, α ≈ 1.2.