| Rapid formation of molecular clouds and stars in the solar neighborhood L Hartmann, J Ballesteros-Paredes, EA Bergin The Astrophysical Journal 562 (2), 852, 2001 | 726 | 2001 |
| Turbulent flow-driven molecular cloud formation: A solution to the post-T Tauri problem? J Ballesteros-Paredes, L Hartmann, E Vázquez-Semadeni The Astrophysical Journal 527 (1), 285, 1999 | 438 | 1999 |
| Molecular cloud evolution. II. From cloud formation to the early stages of star formation in decaying conditions E Vázquez-Semadeni, GC Gómez, AK Jappsen, J Ballesteros-Paredes, ... The Astrophysical Journal 657 (2), 870, 2007 | 404 | 2007 |
| Clouds as turbulent density fluctuations: implications for pressure confinement and spectral line data interpretation J Ballesteros-Paredes, E Vázquez-Semadeni, J Scalo The Astrophysical Journal 515 (1), 286, 1999 | 289 | 1999 |
| Gravity or turbulence? Velocity dispersion–size relation J Ballesteros-Paredes, LW Hartmann, E Vázquez-Semadeni, F Heitsch, ... Monthly Notices of the Royal Astronomical Society 411 (1), 65-70, 2011 | 260 | 2011 |
| Molecular cloud turbulence and star formation J Ballesteros-Paredes, RS Klessen, MM Mac Low, E Vázquez-Semadeni arXiv preprint astro-ph/0603357, 2006 | 252 | 2006 |
| Global hierarchical collapse in molecular clouds. Towards a comprehensive scenario E Vázquez-Semadeni, A Palau, J Ballesteros-Paredes, GC Gómez, ... Monthly Notices of the Royal Astronomical Society 490 (3), 3061-3097, 2019 | 248 | 2019 |
| Molecular cloud formation behind shock waves EA Bergin, LW Hartmann, JC Raymond, J Ballesteros-Paredes The Astrophysical Journal 612 (2), 921, 2004 | 238 | 2004 |
| Physical versus observational properties of clouds in turbulent molecular cloud models J Ballesteros-Paredes, MM Mac Low The Astrophysical Journal 570 (2), 734, 2002 | 214 | 2002 |
| A holistic scenario of turbulent molecular cloud evolution and control of the star formation efficiency: first tests E Vazquez-Semadeni, J Ballesteros-Paredes, RS Klessen The Astrophysical Journal 585 (2), L131, 2003 | 207 | 2003 |
| Formation of molecular clouds and global conditions for star formation CL Dobbs, MR Krumholz, J Ballesteros-Paredes, AD Bolatto, Y Fukui, ... Protostars and Planets VI 1312, 3-26, 2014 | 195 | 2014 |
| The lifetimes and evolution of molecular cloud cores E Vázquez-Semadeni, J Kim, M Shadmehri, J Ballesteros-Paredes The Astrophysical Journal 618 (1), 344, 2005 | 189 | 2005 |
| Gravity or turbulence?–II. Evolving column density probability distribution functions in molecular clouds J Ballesteros-Paredes, E Vázquez-Semadeni, A Gazol, LW Hartmann, ... Monthly Notices of the Royal Astronomical Society 416 (2), 1436-1442, 2011 | 187 | 2011 |
| High-and low-mass star-forming regions from hierarchical gravitational fragmentation. High local star formation rates with low global efficiencies E Vázquez-Semadeni, GC Gómez, AK Jappsen, J Ballesteros-Paredes, ... The Astrophysical Journal 707 (2), 1023, 2009 | 170 | 2009 |
| Protostars and Planets V J Ballesteros-Paredes, RS Klessen, MM Mac Low, E Vazquez-Semadeni, ... University of Arizona Press (arXiv: 0603357), 2007 | 169 | 2007 |
| Quiescent and coherent cores from gravoturbulent fragmentation RS Klessen, J Ballesteros-Paredes, E Vázquez-Semadeni, ... The Astrophysical Journal 620 (2), 786, 2005 | 164 | 2005 |
| Dynamic cores in hydrostatic disguise J Ballesteros-Paredes, RS Klessen, E Vázquez-Semadeni The Astrophysical Journal 592 (1), 188, 2003 | 157 | 2003 |
| Six myths on the virial theorem for interstellar clouds J Ballesteros-Paredes Monthly Notices of the Royal Astronomical Society 372 (1), 443-449, 2006 | 152 | 2006 |
| Molecular cloud evolution. III. Accretion versus stellar feedback E Vázquez-Semadeni, P Colin, GC Gómez, J Ballesteros-Paredes, ... The Astrophysical Journal 715 (2), 1302, 2010 | 148 | 2010 |
| A search for Larson-type relations in numerical simulations of the ISM: Evidence for nonconstant column densities E Vázquez-Semadeni, J Ballesteros-Paredes, LF Rodríguez The Astrophysical Journal 474 (1), 292, 1997 | 142 | 1997 |
Ralf KlessenHeidelberg University在 uni-heidelberg.de 的电子邮件经过验证
