M
Mario Flock
Researcher at Max Planck Society
Publications - 72
Citations - 2705
Mario Flock is an academic researcher from Max Planck Society. The author has contributed to research in topics: Protoplanetary disk & Radiative transfer. The author has an hindex of 24, co-authored 63 publications receiving 2187 citations. Previous affiliations of Mario Flock include University of Paris & Paris Diderot University.
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Journal ArticleDOI
Discovery of a planetary-mass companion within the gap of the transition disk around PDS 70
Miriam Keppler,Myriam Benisty,Myriam Benisty,André Müller,Th. Henning,R. van Boekel,Faustine Cantalloube,Christian Ginski,Christian Ginski,R. G. van Holstein,Anne-Lise Maire,Adriana Pohl,Matthias Samland,Henning Avenhaus,Jean-Loup Baudino,Anthony Boccaletti,J. de Boer,M. Bonnefoy,Gael Chauvin,Gael Chauvin,Silvano Desidera,Maud Langlois,Maud Langlois,C. Lazzoni,G.-D. Marleau,G.-D. Marleau,Christoph Mordasini,N. Pawellek,N. Pawellek,Tomas Stolker,Arthur Vigan,Alice Zurlo,Alice Zurlo,Tilman Birnstiel,Wolfgang Brandner,M. Feldt,Mario Flock,Mario Flock,Mario Flock,Julien Girard,Julien Girard,Raffaele Gratton,Janis Hagelberg,Andrea Isella,Markus Janson,Markus Janson,Attila Juhasz,J. Kemmer,Quentin Kral,Quentin Kral,Anne-Marie Lagrange,Ralf Launhardt,Alexis Matter,Francois Menard,Julien Milli,P. Mollière,Johan Olofsson,Johan Olofsson,Laura M. Pérez,Paola Pinilla,Christophe Pinte,Christophe Pinte,Christophe Pinte,Sascha P. Quanz,T. Schmidt,Stéphane Udry,Zahed Wahhaj,Jonathan Williams,Esther Buenzli,M. Cudel,Carsten Dominik,Raphaël Galicher,M. Kasper,J. Lannier,Dino Mesa,Dino Mesa,David Mouillet,S. Peretti,C. Perrot,Graeme Salter,E. Sissa,Francois Wildi,L. Abe,Jacopo Antichi,Jean-Charles Augereau,Andrea Baruffolo,Pierre Baudoz,Andreas Bazzon,Jean-Luc Beuzit,P. Blanchard,S. S. Brems,Tristan Buey,V. De Caprio,Marcel Carbillet,M. Carle,Enrico Cascone,A. Cheetham,Riccardo Claudi,Anne Costille,A. Delboulbe,Kjetil Dohlen,Daniela Fantinel,Philippe Feautrier,Thierry Fusco,Enrico Giro,L. Gluck,Cecile Gry,Norbert Hubin,Emmanuel Hugot,M. Jaquet,D. Le Mignant,M. Llored,F. Madec,Yves Magnard,Patrice Martinez,D. Maurel,Michael Meyer,Michael Meyer,O. Möller-Nilsson,Thibaut Moulin,Laurent M. Mugnier,Alain Origne,A. Pavlov,D. Perret,Cyril Petit,J. Pragt,Pascal Puget,P. Rabou,Joany Andreina Manjarres Ramos,F. Rigal,S. Rochat,Ronald Roelfsema,Gérard Rousset,A. Roux,Bernardo Salasnich,Jean-François Sauvage,Arnaud Sevin,Christian Soenke,Eric Stadler,M. Suarez,Massimo Turatto,L. Weber +141 more
TL;DR: In this article, the authors detect a point source within the gap of the transition disk at about 195 mas (~22 au) projected separation and detect a signal from an inner disk component.
Journal ArticleDOI
Trapping solids at the inner edge of the dead zone: 3-D global MHD simulations
TL;DR: In this article, a 3D global non-ideal magnetohydrodynamical (MHD) calculation of a section of the disk treating the turbulence driven by the magneto-rotational instability (MRI) was performed.
Journal ArticleDOI
Can dead zones create structures like a transition disk
TL;DR: In this paper, the authors investigated the gas and dust evolution simultaneously assuming simplified prescriptions for a dead zone and a magnetohydrodynamic (MHD) wind acting on the disk.
Journal ArticleDOI
Trapping Solids at the Inner Edge of the Dead Zone: 3-D Global MHD Simulations
TL;DR: In this article, a 3D global non-ideal MHD calculation of the disk was performed, treating the turbulence driven by the magneto-rotational instability. Butterfly pattern was observed in the outer midplane dead zone, with the transition between the two modeled by a sharp increase in the magnetic diffusivity.
Journal ArticleDOI
The vla view of the hl tau disk: disk mass, grain evolution, and early planet formation
Carlos Carrasco-González,Thomas Henning,Claire J. Chandler,Hendrik Linz,Laura M. Pérez,Laura M. Pérez,Luis F. Rodríguez,Roberto Galván-Madrid,Guillem Anglada,Til Birnstiel,Roy van Boekel,Mario Flock,Hubert Klahr,Enrique Macías,Karl Menten,Mayra Osorio,Leonardo Testi,Leonardo Testi,José M. Torrelles,Zhaohuan Zhu +19 more
TL;DR: In this article, the first long-baseline ALMA campaign resolved the disk around the young star HL Tau into a number of axisymmetric bright and dark rings, but the emission from these regions in HL Tau turned out to be optically thick, preventing the derivation of surface density profiles and grain size distributions.