{"id":8,"date":"2018-08-16T12:04:33","date_gmt":"2018-08-16T10:04:33","guid":{"rendered":"http:\/\/valeskavaldivia.space\/?page_id=8"},"modified":"2023-11-14T02:55:23","modified_gmt":"2023-11-14T01:55:23","slug":"publications","status":"publish","type":"page","link":"https:\/\/valeskavaldivia.space\/?page_id=8","title":{"rendered":"Publications"},"content":{"rendered":"<h2><strong>Publications in peer-reviewed scientific journals<\/strong><\/h2>\n<ul>\n<li>\n<h4><strong><span style=\"color: #008080;\"><em>Physical conditions for dust grain alignment in Class 0 protostellar cores II. The role of the radiation field in models aligning\/disrupting dust grains<\/em><\/span><\/strong><\/h4>\n<\/li>\n<\/ul>\n<h5 style=\"padding-left: 40px;\">V. J. M. Le Gouellec, A. J. Maury, C. L. H. Hull, A. Verliat, P. Hennebelle, &amp; <strong>V. Valdivia<\/strong>, <a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2023arXiv230312275L\/abstract\">2023, A&amp;A, 675, 133<\/a><a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2020A%26A...644A..11L\/abstract\">.<\/a><\/h5>\n<ul>\n<li>\n<h4><strong><span style=\"color: #008080;\"><em>3D chemical structure of the diffuse turbulent interstellar medium. II. The origin of CH+: A new solution to an 80-year mystery<\/em><\/span><\/strong><\/h4>\n<\/li>\n<\/ul>\n<h5 style=\"padding-left: 40px;\">B. Godard, G. Pineau des For\u00eats, P. Hennebelle, E. Bellomi, &amp; <strong>V. Valdivia<\/strong>, <a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2023A%26A...669A..74G\/abstract\">2023, A&amp;A, 669, 74<\/a><a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2020A%26A...644A..11L\/abstract\">.<\/a><\/h5>\n<ul>\n<li>\n<h4><span style=\"color: #008080;\"><strong><em>Is the mm\/submm dust polarization a robust tracer of the magnetic field topology in protostellar envelopes? A model exploration<\/em><\/strong><\/span><\/h4>\n<\/li>\n<\/ul>\n<h5 style=\"padding-left: 40px;\"><strong>V. Valdivia<\/strong>, A. J. Maury, &amp; P. Hennebelle, <a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2022A%26A...668A..83V\/abstract\">2022, A&amp;A, 668, 83<\/a><a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2020A%26A...644A..11L\/abstract\">.<\/a><\/h5>\n<ul>\n<li>\n<h4><span style=\"color: #008080;\"><strong><em>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<\/em><\/strong><\/span><\/h4>\n<\/li>\n<\/ul>\n<h5 style=\"padding-left: 40px;\">A. M. Jacob, D. A. Neufeld, P. Schalke, H. Wiesemeyer, W.-J. Kim, S. Bialy, M. Busch, D. Elia, E. Falgarone, M. Gerin, B. Godard, R. Higgins, P. Hennebelle, N. Indriolo, D. C. Lis, K. M. Menten, A. Sanchez-Monge, T. M\u00f6ller, V. Ossenkopf-Okada, M. R. Rugel, D. Seifried, P. Sonnentrucker, S. Walch, M. G. Wolfire, F. Wyrowski, F., &amp; <strong>V. Valdivia<\/strong>, <a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2022ApJ...930..141J\/abstract\">2022, ApJ, 930, 141<\/a><a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2020A%26A...644A..11L\/abstract\">.<\/a><\/h5>\n<ul>\n<li>\n<h4><strong><span style=\"color: #008080;\"><em>Calibrating the Davis-Chandrasekhar-Fermi Method with Numerical Simulations: Uncertainties in Estimating the Magnetic Field Strength from Statistics of Field Orientations<\/em><\/span><\/strong><\/h4>\n<\/li>\n<\/ul>\n<h5 style=\"padding-left: 40px;\">J. Liu, Q. Zhang, B. Commer\u00e7on, <strong>V. Valdivia<\/strong>, A. J. Maury, &amp; K. Qiu, <a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2021ApJ...919...79L\/abstract\">2021, ApJ, 919, 79<\/a><a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2020A%26A...644A..11L\/abstract\">.<\/a><\/h5>\n<ul>\n<li>\n<h4><span style=\"color: #008080;\"><strong><em>An observational correlation between magnetic field, angular momentum and fragmentation in the envelopes of Class 0 protostars?<\/em><\/strong><\/span><\/h4>\n<\/li>\n<\/ul>\n<h5 style=\"padding-left: 40px;\">M. Galametz, A. J. Maury, J. M. Girart, R. Rao, Q. Zhang, M. Gaudel, <strong>V. Valdivia<\/strong>, P. Hennebelle, V. Cabedo-Soto, E. Keto,\u00a0&amp; S-P. Lai, <a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2020A%26A...644A..47G\/abstract\">2020, A&amp;A, 644, A47<\/a><a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2020A%26A...644A..11L\/abstract\">.<\/a><\/h5>\n<ul>\n<li>\n<h4><span style=\"color: #008080;\"><strong><em>A statistical analysis of dust polarization properties in ALMA observations of Class 0 protostellar cores<\/em><\/strong><\/span><\/h4>\n<\/li>\n<\/ul>\n<h5 style=\"padding-left: 40px;\">V. J. M. Le Gouellec, A. J. Maury, V. Guillet, C. L. H. Hull, J. M. Girart, A. Verliat, R. Mignon-Risse, <strong>V. Valdivia<\/strong>, P. Hennebelle, M. Gonz\u00e1lez, &amp; F. Louvet, <a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2020A%26A...644A..11L\/abstract\">2020, A&amp;A, 644, A11<\/a><a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2020A%26A...644A..11L\/abstract\">.<\/a><\/h5>\n<ul>\n<li>\n<h4><span style=\"color: #008080;\"><strong><em>3D chemical structure of diffuse turbulent ISM. I. Statistics of the HI-to-H2 transition<\/em><\/strong><\/span><\/h4>\n<\/li>\n<\/ul>\n<h5 style=\"padding-left: 40px;\">E. Bellomi, B. Godard, P. Hennebelle, <strong>V. Valdivia<\/strong>, G. Pineau des For\u00eats, P. Lesaffre, &amp; M. P\u00e9rault, <a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2020A%26A...643A..36B\/abstract\">2020, A&amp;A, 643, A36.<\/a><\/h5>\n<ul>\n<li>\n<h4><span style=\"color: #008080;\"><strong><em>Production and excitation of molecules by dissipation of two-dimensional turbulence<\/em><\/strong><\/span><\/h4>\n<\/li>\n<\/ul>\n<h5 style=\"padding-left: 40px;\">P. Lesaffre, P. Todorov, F. Levrier, <strong>V. Valdivia<\/strong>, N. Dzyurkevich, B. Godard, L. N. Tram, A. Gusdorf, A. Lehmann, &amp; E. Falgarone, <a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2020MNRAS.495..816L\/abstract\">2020, MNRAS, 495, 816.<\/a><\/h5>\n<ul>\n<li>\n<h4><span style=\"color: #008080;\"><strong><em>Low dust emissivities and radial variations in the envelopes of Class 9 protostars: possible signature of early grain growth<\/em><\/strong><\/span><\/h4>\n<\/li>\n<\/ul>\n<h5 style=\"padding-left: 40px;\">M. Galametz, A. J. Maury, <strong>V. Valdivia<\/strong>, L. Testi, A. Belloche &amp; Ph. Andr\u00e9,\u00a0<a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2019A%26A...632A...5G\/abstract\">2019, A&amp;A, 632, A5.<\/a><\/h5>\n<ul>\n<li>\n<h4><span style=\"color: #008080;\"><strong><em>Indirect evidence of significant grain growth in young protostellar envelopes from polarized dust emission<\/em><\/strong><\/span><\/h4>\n<\/li>\n<\/ul>\n<h5 style=\"padding-left: 40px;\"><strong>V. Valdivia,\u00a0<\/strong>A. Maury, R. Brauer, P. Hennebelle, M. Galametz, V. Guillet,\u00a0&amp; S. Reissl,\u00a0<a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2019MNRAS.488.4897V\/abstract\">2019, MNRAS, 488, 4897-4904.<\/a><\/h5>\n<ul>\n<li><span style=\"color: #008080;\"><strong><em>SMA observations of the polarized dust emission in solar-type Class 0 protostars: Magnetic field properties at\u00a0envelope scales<\/em><\/strong><\/span><\/li>\n<\/ul>\n<h5 style=\"padding-left: 40px;\">M. Galametz, A. Maury, J-M. Girart, R. Rao, Q. Zhang, M. Gaudel, <strong>V. Valdivia<\/strong>, E. Keto, &amp; S-P. Lai,\u00a0<a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2018A%26A...616A.139G\/abstract\">2018, A&amp;A, 616, A139.<\/a><\/h5>\n<ul>\n<li><span style=\"color: #008080;\"><strong>\u00a0<em>H2 formation on interstellar dust grains: the viewpoints of theory, experiments, models and observations<\/em><\/strong><\/span><\/li>\n<\/ul>\n<h5 style=\"padding-left: 40px;\">V. Wakelam, E. Bron, S. Cazaux, F. Dulieu, C. Gry, P. Guillard, E. Habart, L. Hornek\u00e6r, S. Morisset, G.\u00a0Nyman, S. Price, V. Pirronello, <strong>V. Valdivia<\/strong>, G. Vidali, &amp; N. Watanabe,\u00a0<a href=\"http:\/\/adsabs.harvard.edu\/abs\/2017MolAs...9....1W\">2017, Molecular Astrophysics, 9, 1<\/a><\/h5>\n<ul>\n<li>\n<h4><strong style=\"color: #008080; font-size: revert;\"><em>Origin of CH+ in diffuse molecular clouds warm H2 and ion-neutral drift<\/em><\/strong><\/h4>\n<\/li>\n<\/ul>\n<h5 style=\"padding-left: 40px;\"><strong>V. Valdivia<\/strong>, B. Godard, P. Hennebelle, M. Gerin, P. Lesaffre, &amp; J. Le Bourlot,\u00a0<a href=\"http:\/\/adsabs.harvard.edu\/abs\/2017A%26A...600A.114V\">2017, A&amp;A, 600, A114<\/a><\/h5>\n<ul>\n<li>\n<h4><strong style=\"color: #008080; font-size: revert;\"><em>H2 distribution during the formation of multiphase molecular clouds<\/em><\/strong><\/h4>\n<\/li>\n<\/ul>\n<h5 style=\"padding-left: 40px;\"><strong>V. Valdivia<\/strong>, P. Hennebelle, M. Gerin, &amp; P. Lesaffre,\u00a0<a href=\"http:\/\/adsabs.harvard.edu\/abs\/2016A%26A...587A..76V\">2016, A&amp;A, 587, A76<\/a><\/h5>\n<ul>\n<li>\n<h4><span style=\"color: #008080;\"><strong><em>A fast tree-based method for estimating column densities in adaptive mesh refinement codes. Influence of UV\u00a0radiation field on the structure of molecular clouds<\/em><\/strong><\/span><\/h4>\n<\/li>\n<\/ul>\n<h5 style=\"padding-left: 40px;\"><strong>V. Valdivia<\/strong> &amp; P. Hennebelle,\u00a0<a href=\"http:\/\/adsabs.harvard.edu\/abs\/2014A%26A...571A..46V\">2014, A&amp;A, 571, A46<\/a><\/h5>\n<h2><strong>Conference papers<\/strong><\/h2>\n<ul>\n<li><em>\u00a0Chemical Evolution of Turbulent Multiphase Molecular Clouds.<\/em><\/li>\n<\/ul>\n<p><span style=\"font-size: 1rem;\">Authors : <\/span><strong style=\"font-size: 1rem;\">V. Valdivia<\/strong><span style=\"font-size: 1rem;\">, P. Hennebelle, B. Godard, M. Gerin, P. Lesaffre, &amp; J. Le Bourlot, \u00a0<\/span><a style=\"font-size: 1rem;\" href=\"http:\/\/adsabs.harvard.edu\/abs\/2018IAUS..332..242V\">Proceedings of IAU S332: Astrochemistry VII \u2013 Through the Cosmos from\u00a0Galaxies to Planets. Eds.: Maria Cunningham, Tom Millar and Yuri Aikawa<\/a><\/p>\n<ul>\n<li><em>\u00a0Consequences of warm H2 on the chemistry of diffuse molecular clouds: the case of CH+.<\/em><\/li>\n<\/ul>\n<p>Authors : <strong>V. Valdivia<\/strong>, B. Godard, P. Hennebelle, M. Gerin, &amp; P. Lesaffre, \u00a0<a href=\"http:\/\/adsabs.harvard.edu\/abs\/2016sf2a.conf..309V\">SF2A-2016: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics. Eds.: C.\u00a0Reyl\u00e9, J. Richard, L. Cambr\u00e9sy, M. Deleuil, E. P\u00e9contal, L. Tresse and I. Vauglin, held 14-17 June, 2016 at the\u00a0Centre de Recherche Astrophysique de Lyon, pp.309-313<\/a><\/p>\n<ul>\n<li><em>\u00a0Chemistry and dynamics: a post-processing tool towards a real coupling.<\/em><\/li>\n<\/ul>\n<p>Authors : <strong>V. Valdivia<\/strong>, B. Godard, P. Hennebelle, M. Gerin, &amp; P. Lesaffre, \u00a0<a href=\"http:\/\/adsabs.harvard.edu\/abs\/2016sf2a.conf..163V\">SF2A-2016: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics. Eds.: C.\u00a0Reyl\u00e9, J. Richard, L. Cambr\u00e9sy, M. Deleuil, E. P\u00e9contal, L. Tresse and I. Vauglin, held 14-17 June, 2016 at the\u00a0Centre de Recherche Astrophysique de Lyon, pp.163-167<\/a><\/p>\n<ul>\n<li><em>\u00a0H2 Distribution during 2-phase Molecular Cloud Formation<\/em><\/li>\n<\/ul>\n<p>Authors : <strong>V. Valdivia<\/strong>, P. Hennebelle, M. Gerin, P. Lesaffre, \u00a0<a href=\"http:\/\/adsabs.harvard.edu\/abs\/2015EAS....75..393V\">Conditions and Impact of Star Formation. Edited by R. Simon, R. Schaaf and J. Stutzki. EAS Publications Series,\u00a0Volume 75-76, 2015, pp.393-394<\/a><\/p>\n","protected":false},"excerpt":{"rendered":"<p>Publications in peer-reviewed scientific journals Physical conditions for dust grain alignment in Class 0 protostellar cores II. The role of the radiation field in models aligning\/disrupting dust grains V. J. M. Le Gouellec, A. J. Maury, C. L. H. Hull, A. Verliat, P. Hennebelle, &amp; V. Valdivia, 2023, A&amp;A, 675, 133. 3D chemical structure of&#8230;<\/p>\n","protected":false},"author":1,"featured_media":90,"parent":0,"menu_order":4,"comment_status":"closed","ping_status":"closed","template":"","meta":{"footnotes":""},"class_list":["post-8","page","type-page","status-publish","has-post-thumbnail","hentry"],"_links":{"self":[{"href":"https:\/\/valeskavaldivia.space\/index.php?rest_route=\/wp\/v2\/pages\/8","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/valeskavaldivia.space\/index.php?rest_route=\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/valeskavaldivia.space\/index.php?rest_route=\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/valeskavaldivia.space\/index.php?rest_route=\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/valeskavaldivia.space\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=8"}],"version-history":[{"count":39,"href":"https:\/\/valeskavaldivia.space\/index.php?rest_route=\/wp\/v2\/pages\/8\/revisions"}],"predecessor-version":[{"id":254,"href":"https:\/\/valeskavaldivia.space\/index.php?rest_route=\/wp\/v2\/pages\/8\/revisions\/254"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/valeskavaldivia.space\/index.php?rest_route=\/wp\/v2\/media\/90"}],"wp:attachment":[{"href":"https:\/\/valeskavaldivia.space\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=8"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}