activity
20162020
most citedAre fibres in molecular cloud filaments real objects?

48 citations · 122 across the 3 of their papers we have counts for

collaborators

8 papers

astro-ph.GA2020

Simultaneous evolution of the virial parameter and star formation rate in molecular clumps undergoing global hierarchical collapse

Vianey Camacho, Enrique Vázquez-Semadeni, Aina Palau +2

We compare dense clumps and cores in a numerical simulation of molecular clouds (MCs) undergoing global hierarchical collapse (GHC) to observations in two MCs at different evolutio…

astro-ph.SR2019

Flipping-up the field: gravitational feedback as a mechanism for young clusters dispersal

Manuel Zamora-Avilés, Javier Ballesteros-Paredes, Jesús Hernández +3

Recent analyses of Gaia data have provided direct evidence that most young stellar clusters are in a state of expansion, with velocities of the order of ~0.5 km/s. Traditionally, e…

astro-ph.GA2019

Global Hierarchical Collapse In Molecular Clouds. Towards a Comprehensive Scenario

Enrique Vázquez-Semadeni, Aina Palau, Javier Ballesteros-Paredes +2

We present a unified description of the scenario of Global Hierarchical Collapse and fragmentation (GHC) in molecular clouds (MCs), owing to the continuous decrease of the average…

astro-ph.GA201939 cited

Structure and Expansion Law of HII Regions in structured Molecular Clouds

Manuel Zamora-Avilés, Enrique Vázquez-Semadeni, Ricardo F. González +6

We present radiation-magnetohydrodynamic simulations aimed at studying evolutionary properties of H\,{\normalsize II} regions in turbulent, magnetised, and collapsing molecular clo…

astro-ph.GA2018

Molecular Cloud Evolution VI. Measuring cloud ages

Enrique Vázquez-Semadeni, Manuel Zamora-Avilés, Roberto Galván-Madrid +1

In previous contributions, we have presented an analytical model describing the evolution of molecular clouds (MCs) undergoing hierarchical gravitational contraction. The cloud's e…

astro-ph.GA201748 cited

Are fibres in molecular cloud filaments real objects?

Manuel Zamora-Avilés, Javier Ballesteros-Paredes, Lee W. Hartmann

We analyse the morphology and kinematics of dense filamentary structures produced in a numerical simulation of a star--forming cloud of $1.4 \times 10^4 \, \Msun$ evolving under th…