| Gravity or turbulence?–III. Evidence of pure thermal Jeans fragmentation at∼ 0.1 pc scale A Palau, J Ballesteros-Paredes, E Vázquez-Semadeni, ... Monthly Notices of the Royal Astronomical Society 453 (4), 3785-3797, 2015 | 90 | 2015 |
| Energy budget of forming clumps in numerical simulations of collapsing clouds V Camacho, E Vázquez-Semadeni, J Ballesteros-Paredes, GC Gómez, ... The Astrophysical Journal 833 (1), 113, 2016 | 39 | 2016 |
| Simultaneous evolution of the virial parameter and star formation rate in molecular clumps undergoing global hierarchical collapse V Camacho, E Vázquez-Semadeni, A Palau, G Busquet, M Zamora-Avilés The Astrophysical Journal 903 (1), 46, 2020 | 14 | 2020 |
| Why most molecular clouds are gravitationally dominated L Ramírez-Galeano, J Ballesteros-Paredes, RJ Smith, V Camacho, ... Monthly Notices of the Royal Astronomical Society 515 (2), 2822-2836, 2022 | 10 | 2022 |
| Gravity or turbulence V: star-forming regions undergoing violent relaxation A Bonilla-Barroso, J Ballesteros-Paredes, J Hernández, L Aguilar, ... Monthly Notices of the Royal Astronomical Society 511 (4), 4801-4814, 2022 | 8 | 2022 |
| The kinetic and magnetic energy budget of hub-filament systems during the gravitational fragmentation of molecular clouds V Camacho, E Vázquez-Semadeni, A Palau, M Zamora-Avilés Monthly Notices of the Royal Astronomical Society 523 (3), 3376-3392, 2023 | 3 | 2023 |
| Simultaneous evolution of the virial parameter and star formation rate in star forming molecular clouds V Camacho, E Vázquez-Semadeni, A Palau, G Busquet, M Zamora-Avilés arXiv e-prints, arXiv: 2002.01594, 2020 | | 2020 |
