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Author

Valeska Valdivia

Observed names: V Valdivia, V. Valdivia, Valdivia, V., Valdivia, Valeska
Institution: Nagoya University
Observed institutions: Centre National de la Recherche Scientifique, Commissariat à l'Énergie Atomique et aux Énergies Alternatives, Université Paris Sciences et Lettres, Université Paris-Saclay, Observatoire de Paris, CEA Paris-Saclay - Etablissement de Saclay, École Normale Supérieure - PSL, Sorbonne Université, Astrophysique, Instrumentation et Modélisation, Sorbonne Paris Cité, Laboratoire d’Etudes du Rayonnement et de la Matière en Astrophysique et Atmosphères, CEA Paris-Saclay, Institut de Recherche sur les Lois Fondamentales de l'Univers, Université Paris Diderot, Université Pierre-et-Marie-Curie, Nagoya University
ORCID: 0000-0002-5595-822X
Observed ORCID: 0000-0002-5595-822X
OpenAlex ID: A5033483825
H 2 formation on interstellar dust grains: The viewpoints of theory, experiments, models and observations
2017 · Valentine Wakelam, Emeric Bron, et al. · Molecular astrophysics · 288
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Low dust emissivities and radial variations in the envelopes of Class 0 protostars: possible signature of early grain growth
2019 · M. Galametz, A. J. Maury, et al. · Astronomy and Astrophysics · 104
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H2distribution during the formation of multiphase molecular clouds
2015 · Valeska Valdivia, Patrick Hennebelle, et al. · Astronomy and Astrophysics · 78
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Calibrating the Davis–Chandrasekhar–Fermi Method with Numerical Simulations: Uncertainties in Estimating the Magnetic Field Strength from Statistics of Field Orientations
2021 · Junhao 峻豪 Liu 刘, Qizhou Zhang, et al. · The Astrophysical Journal · 63
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SMA observations of polarized dust emission in solar-type Class 0 protostars: Magnetic field properties at envelope scales
2018 · Maud Galametz, Anaëlle Maury, et al. · Astronomy and Astrophysics · 58
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3D chemical structure of diffuse turbulent ISM: I. Statistics of the HI-to-H2 transition
2020 · E. Bellomi, B. Godard, et al. · Astronomy and Astrophysics · 54
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Indirect evidence of significant grain growth in young protostellar envelopes from polarized dust emission
2019 · Valeska Valdivia, Anaëlle Maury, et al. · Monthly Notices of the Royal Astronomical Society · 53
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SMA observations of polarized dust emission in solar-type Class 0 protostars: Magnetic field properties at envelope scales
2018 · Maud Galametz, Anaëlle Maury, et al. · Springer Link (Chiba Institute of Technology) · 50
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A statistical analysis of dust polarization properties in ALMA observations of Class 0 protostellar cores
2020 · V. J. M. Le Gouellec, A. J. Maury, et al. · Astronomy and Astrophysics · 46
Origin of CH+ in diffuse molecular clouds: Warm H2 and ion-neutral drift
2016 · Valeska Valdivia, Benjamin Godard, et al. · Astronomy and Astrophysics · 42
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An observational correlation between magnetic field, angular momentum and fragmentation in the envelopes of Class 0 protostars?
2020 · Maud Galametz, Anaëlle Maury, et al. · Astronomy and Astrophysics · 29
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3D chemical structure of the diffuse turbulent interstellar medium: II. The origin of CH + : A new solution to an 80-year mystery
2022 · B. Godard, G. Pineau des Forêts, et al. · Astronomy and Astrophysics · 23
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HyGAL: Characterizing the Galactic Interstellar Medium with Observations of Hydrides and Other Small Molecules. I. Survey Description and a First Look Toward W3(OH), W3 IRS5, and NGC 7538 IRS1
2022 · A. M. Jacob, D. A. Neufeld, et al. · The Astrophysical Journal · 22
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Production and excitation of molecules by dissipation of two-dimensional turbulence
2020 · P Lesaffre, P Todorov, et al. · Monthly Notices of the Royal Astronomical Society · 20
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A fast tree-based method for estimating column densities in adaptive mesh refinement codes: Influence of UV radiation field on the structure of molecular clouds
2014 · Valeska Valdivia, Patrick Hennebelle · Astronomy and Astrophysics · 14
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Is the mm/submm dust polarization a robust tracer of the magnetic field topology in protostellar envelopes? A model exploration
2022 · Valeska Valdivia, Anaëlle Maury, et al. · Astronomy and Astrophysics · 13
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Physical conditions for dust grain alignment in Class 0 protostellar cores: II. The role of the radiation field in models that align and disrupt dust grains
2023 · V. J. M. Le Gouellec, A. J. Maury, et al. · Astronomy and Astrophysics · 10
ESA Voyage 2050 white paper: A complete census of the gas phases in and around galaxies, far-UV spectropolarimetry as a prime tool for understanding galaxy evolution and star formation
2019 · Lebouteiller, V., Yan, C. Gry. H., et al. · arXiv (Cornell University) · 2
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Chemical Evolution of Turbulent Multiphase Molecular Clouds
2017 · Valeska Valdivia, Patrick Hennebelle, et al. · Proceedings of the International Astronomical Union · 2
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H2Distribution during 2-phase Molecular Cloud Formation
2015 · V. Valdivia, P. Hennebelle, et al. · EAS Publications Series · 2
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Towards Realistic Predictions Of Mm/Sub-Mm Polarized Dust Emission
2017 · Valdivia, Valeska, Maury, A., et al. · 1
HyGAL. III. Absorption lines
2026 · Kim, W.-J., Jacob, A. M., et al. · Strasbourg Astronomical Data Center
HyGAL. III. Absorption lines : J/A+A/710/A301 [Dataset]
2026 · Kim, Won-Ju, Jacob, A. M., et al. · DIGITAL.CSIC (Spanish National Research Council (CSIC))
HyGAL: Characterizing the Galactic ISM with observations of hydrides and other small molecules
2026 · W.-J. Kim, A. M. Jacob, et al. · Astronomy and Astrophysics
Dissecting the dust distribution and polarization around two B213 young stellar objects with ALMA
2026 · Asako Sato, Anaëlle Maury, et al. · Astronomy and Astrophysics
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Works count: 41
Citation count: 975
H-index: 14
I10-index: 17
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