| What happens when n= 1000? Creating large-n geochronological datasets with LA-ICP-MS for geologic investigations A Pullen, M Ibáñez-Mejía, GE Gehrels, JC Ibáñez-Mejía, M Pecha Journal of Analytical Atomic Spectrometry 29 (6), 971-980, 2014 | 225 | 2014 |
| Modelling the supernova-driven ISM in different environments A Gatto, S Walch, MMM Low, T Naab, P Girichidis, SCO Glover, R Wünsch, ... Monthly Notices of the Royal Astronomical Society 449 (1), 1057-1075, 2015 | 171 | 2015 |
| Use and abuse of detrital zircon U-Pb geochronology—A case from the Río Orinoco delta, eastern Venezuela M Ibañez-Mejia, A Pullen, M Pepper, F Urbani, G Ghoshal, ... Geology 46 (11), 1019-1022, 2018 | 92 | 2018 |
| Gravitational contraction versus supernova driving and the origin of the velocity dispersion–size relation in molecular clouds JC Ibáñez-Mejía, MM Mac Low, RS Klessen, C Baczynski The Astrophysical Journal 824 (1), 41, 2016 | 83 | 2016 |
| SILCC-Zoom: Polarization and depolarization in molecular clouds D Seifried, S Walch, S Reissl, JC Ibáñez-Mejía Monthly Notices of the Royal Astronomical Society 482 (2), 2697-2716, 2019 | 45 | 2019 |
| Feeding versus Falling: The Growth and Collapse of Molecular Clouds in a Turbulent Interstellar Medium JC Ibáñez-Mejía, MM Mac Low, RS Klessen, C Baczynski The Astrophysical Journal 850 (1), 62, 2017 | 38 | 2017 |
| Effect of the Heating Rate on the Stability of the Three-phase Interstellar Medium AS Hill, MM Mac Low, A Gatto, JC Ibáñez-Mejía The Astrophysical Journal 862 (1), 55, 2018 | 32 | 2018 |
| On the fragmentation of filaments in a molecular cloud simulation RA Chira, J Kainulainen, JC Ibáñez-Mejía, T Henning, MM Mac Low Astronomy & Astrophysics 610, A62, 2018 | 25 | 2018 |
| Dust charge distribution in the interstellar medium JC Ibáñez-Mejía, S Walch, AV Ivlev, S Clarke, P Caselli, PR Joshi Monthly Notices of the Royal Astronomical Society 485 (1), 1220-1247, 2019 | 19 | 2019 |
| Determining the presence of characteristic fragmentation length-scales in filaments SD Clarke, GM Williams, JC Ibáñez-Mejía, S Walch Monthly Notices of the Royal Astronomical Society 484 (3), 4024-4045, 2019 | 18 | 2019 |
| How do velocity structure functions trace gas dynamics in simulated molecular clouds? RA Chira, JC Ibáñez-Mejía, MM Mac Low, T Henning Astronomy & Astrophysics 630, A97, 2019 | 17 | 2019 |
| Gravity versus Magnetic Fields in Forming Molecular Clouds JC Ibáñez-Mejía, MM Mac Low, RS Klessen The Astrophysical Journal 925 (2), 196, 2022 | 15 | 2022 |
| The catalogue for astrophysical turbulence simulations (cats) B Burkhart, SM Appel, S Bialy, J Cho, AJ Christensen, D Collins, ... The Astrophysical Journal 905 (1), 14, 2020 | 15 | 2020 |
| Fast Molecular Cloud Destruction Requires Fast Cloud Formation MM Mac Low, A Burkert, JC Ibáñez-Mejía The Astrophysical Journal Letters 847 (1), L10, 2017 | 15 | 2017 |
| Stability of toroidal magnetic fields in stellar interiors JC Ibáñez-Mejía, J Braithwaite Astronomy & Astrophysics 578, A5, 2015 | 12 | 2015 |
| Supplemental Data: Effect of the heating rate on the stability of the three-phase interstellar medium AS Hill, MM Mac Low, A Gatto, JC Ibáñez-Mejía Hill et al (2018; arXiv: 1806.05571), 2018 | 2 | 2018 |
| Simulating stellar cluster formation and early evolution J Wall, SLW McMillan, MM Mac Low, J Ibañez-Mejia, S Portegies Zwart, ... American Astronomical Society Meeting Abstracts# 229 229, 153.02, 2017 | 2 | 2017 |
| Use and abuse of detrital zircon U-Pb geochronology—A case from the Río Orinoco delta, eastern Venezuela: Geology M Ibañez-Mejia, A Pullen, M Pepper, F Urbani, G Ghoshal, ... | 1 | 2018 |
| FragMent: Fragmentation techniques for studying filaments SD Clarke, GM Williams, JC Ibáñez-Mejía, S Walch Astrophysics Source Code Library, ascl: 2001.004, 2020 | | 2020 |
| DustCharge: Charge distribution for a dust grain JC Ibáñez-Mejía, S Walch, AV Ivlev, S Clarke, P Caselli, PR Joshi Astrophysics Source Code Library, ascl: 1908.016, 2019 | | 2019 |
Mordecai-Mark Mac LowDept. of Astrophysics, American Museum of Natural HistoryVerified email at amnh.org
