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MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 495(1):L7-L11. 2020 A novel framework for studying the impact of binding energy distributions on the chemistry of dust grains. ASTRONOMY & ASTROPHYSICS. 643. 2020 High level ab initio binding energy distribution of molecules on interstellar ices: Hydrogen fluoride. MOLECULAR ASTROPHYSICS. 21. 2020 Predicting FIR lines from simulated galaxies. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 496(4):5160-5175. 2020 Survey of ortho-H2D+in high-mass star-forming regions. ASTRONOMY & ASTROPHYSICS. 644. 2020 The [C II]-SFR correlation in dwarf galaxies across cosmic time. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 492(2):2818-2827. 2020 A timeline for massive star-forming regions via combined observation of o-H2D+ and N2D+. ASTRONOMY & ASTROPHYSICS. 621:1-7. 2019 Black hole formation in the context of dissipative dark matter. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 485(3):3352-3359. 2019 High-redshift quasars and their host galaxies - I. Kinematical and dynamical properties and their tracers. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 488(3):4004-4022. 2019 On the size of the CO-depletion radius in the IRDC G351.77-0.51. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 490(4):4489-4501. 2019 The 3D Structure of CO Depletion in High-mass Prestellar Regions. ASTROPHYSICAL JOURNAL. 887(2). 2019 Fast deuterium fractionation in magnetized and turbulent filaments. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 478(1):95-109. 2018 The effect of non-equilibrium metal cooling on the interstellar medium. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 475(3):3283-3304. 2018 The formation of protostellar binaries in primordial minihaloes. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 479(1):667-686. 2018 The natural emergence of the correlation between H2 and star formation rate surface densities in galaxy simulations. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 474(3):2884-2903. 2018 H-2 Ortho-to-para Conversion on Grains: A Route to Fast Deuterium Fractionation in Dense Cloud Cores?. ASTROPHYSICAL JOURNAL LETTERS. 849(2):1-6. 2017
Relacionados por A new proxy to estimate the cosmic ray ionization rate in dense cores A novel framework for studying the impact of binding energy distributions on the chemistry of dust grains A timeline for massive star-forming regions via combined observation of o-H2D+ and N2D+ Binding Energy Evaluation Platform: A Database of Quantum Chemical Binding Energy Distributions for the Astrochemical Community Black hole formation in the context of dissipative dark matter CO Diffusion on Interstellar Amorphous Solid Water: A Computational Study Chemical analysis of prestellar cores in Ophiuchus yields short timescales and rapid collapse Chemical post-processing of magneto-hydrodynamical simulations of star-forming regions: robustness and pitfalls Establishing the evolutionary timescales of the massive star formation process through chemistry Fast deuterium fractionation in magnetized and turbulent filaments First ALMA Maps of Cosmic-Ray Ionization Rate in High-mass Star-forming Regions Formation of metal-free binaries: Impact of H2 line cooling and CIE cooling H-2 Ortho-to-para Conversion on Grains: A Route to Fast Deuterium Fractionation in Dense Cloud Cores? High level ab initio binding energy distribution of molecules on interstellar ices: Hydrogen fluoride High-redshift quasars and their host galaxies - I. Kinematical and dynamical properties and their tracers High-redshift quasars and their host galaxies - II. Multiphase gas and stellar kinematics Identification of pre-stellar cores in high-mass star forming clumps via H2D+ observations with ALMA In-depth exploration of catalytic sites on amorphous solid water: I. The astrosynthesis of aminomethanol Modelling H-2 and its effects on star formation using a joint implementation of gadget-3 and KROME Molecular gas properties of Q1700-MD94: A massive main-sequence galaxy at z approximate to 2 Non-ideal magnetohydrodynamics of self-gravitating filaments On the low ortho-to-para H-2 ratio in star-forming filaments On the size of the CO-depletion radius in the IRDC G351.77-0.51 Predicting FIR lines from simulated galaxies Presence of water on exomoons orbiting free-floating planets: a case study Profesor Asociado Profesor guía Reducing the complexity of chemical networks via interpretable autoencoders Survey of ortho-H2D+in high-mass star-forming regions Synthetic observations using POLARIS: an application to simulations of massive prestellar cores The 3D Structure of CO Depletion in High-mass Prestellar Regions The Astrochemistry Low-energy Electron Cross-Section (ALeCS) database I. Semi-empirical electron-impact ionization cross-section calculations and ionization rates The Fermi paradox: impact of astrophysical processes and dynamical evolution The [C II]-SFR correlation in dwarf galaxies across cosmic time The alma survey of 70 mu m dark high-mass clumps in early stages (ashes). vi. the core-scale co depletion The alma survey of 70 mu m dark high-mass clumps in early stages (ashes). vii. chemistry of embedded dense cores The core population and kinematics of a massive clump at early stages: an atacama large millimeter/submillimeter array view The effect of non-equilibrium metal cooling on the interstellar medium The formation of protostellar binaries in primordial minihaloes The natural emergence of the correlation between H2 and star formation rate surface densities in galaxy simulations Time evolution of o-H2D+, N2D+, and N2H+ during the high-mass star formation process Unusually high hco+/co ratios in and outside supernova remnant w49b