Felipe Alarcón
University of Michigan
5 Papers
20 Citations
Felipe Alarcón is an academic researcher from University of Michigan. The author has contributed to research in topics: Protoplanetary disk & Planet. The author has an hindex of 3, co-authored 5 publications.
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Papers
Long Baseline Observations of the HD 100546 Protoplanetary Disk with ALMA
Sebastián Pérez,Sebastián Pérez,Simon Casassus,Antonio Hales,Antonio Hales,Sebastian Marino,Anthony Cheetham,Anthony Cheetham,Alice Zurlo,Lucas A. Cieza,Ruobing Dong,Felipe Alarcón,Pablo Benítez-Llambay,Ed Fomalont,Ed Fomalont,Henning Avenhaus +15 more
TL;DR: Government of Chile grant Millennium Scientific Initiative (MSI) 2017 as mentioned in this paper, and CONICYT-FONDECYT (FondecyT-Gemini) 2017
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Molecules with ALMA at Planet-forming Scales (MAPS). XV. Tracing Protoplanetary Disk Structure within 20 au
Arthur D. Bosman,Edwin A. Bergin,Ryan A. Loomis,Sean M. Andrews,Merel L. R. van ’t Hoff,Richard Teague,Karin I. Öberg,Viviana V. Guzmán,Catherine Walsh,Yuri Aikawa,Felipe Alarcón,Jaehan Bae,Jennifer B. Bergner,Alice S. Booth,Alice S. Booth,Gianni Cataldi,L. Ilsedore Cleeves,Ian Czekala,Jane Huang,Jane Huang,John D. Ilee,Charles J. Law,Romane Le Gal,Yao Liu,Feng Long,Francois Menard,Hideko Nomura,Laura M. Pérez,Chunhua Qi,Kamber R. Schwarz,Anibal Sierra,Takashi Tsukagoshi,Yoshihide Yamato,David J. Wilner,Ke Zhang +34 more
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Chemical Evolution in a Protoplanetary Disk within Planet Carved Gaps and Dust Rings
Felipe Alarcón,Richard Teague,Richard Teague,Ke Zhang,Ke Zhang,Edwin A. Bergin,Marcelo Barraza-Alfaro +6 more
TL;DR: In this paper, the authors use a thermochemical code to focus on the chemical evolution that is occurring within the gas-depleted gap and the dust-rich ring often observed behind it, showing that the dust temperature at the midplane of the gap increases, enough to produce local sublimation of key volatiles and pushing the molecular layer closer to the mid plane, while it decreases in the dustrich ring, causing a higher volatile deposition onto the dust grain surfaces.
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•Posted Content
Planet formation: The case for large efforts on the computational side
Wladimir Lyra,Thomas J. Haworth,Bertram Bitsch,Simon Casassus,Nicolás Cuello,Thayne Currie,Andras Gaspar,Hannah Jang-Condell,Hubert Klahr,Nathan Leigh,Giuseppe Lodato,Mordecai-Mark Mac Low,Sarah T. Maddison,George Mamatsashvili,Colin P. McNally,Andrea Isella,Sebastian Perez,Luca Ricci,Debanjan Sengupta,Dimitris Stamatellos,Judit Szulágyi,Richard Teague,Neal J. Turner,Orkan M. Umurhan,Jacob Aaron White,A. Wootten,Felipe Alarcón,Daniel Apai,Amelia Bayo,Edwin A. Bergin,Daniel Carrera,Ilse Cleeves,Asantha Cooray,Gregor J. Golabek,Oliver Gressel,Mark Gurwell,Sebastiaan Krijt,Cassandra Hall,Ruobing Dong,Fujun Du,Ilaria Pascucci,John D. Ilee,Andre Izidoro,Jes K. Jørgensen,Mihkel Kama,Dimitri Mawet,Jinyoung Serena Kim,David Leisawitz,Tim Lichtenberg,Nienke van der Marel,Margaret Meixner,John D. Monnier,Giovanni Picogna,Klaus M. Pontoppidan,Hsien Shang,Jake Simon,David J. Wilner +56 more
TL;DR: In this paper, the authors identified the nature of accretion, ab initio planet formation, early evolution, and circumplanetary disks as major fields of interest in computational planet formation and recommended that modelers relax the approximations of alpha-viscosity and isothermal equations of state.
Chemical Evolution in a Protoplanetary Disk within Planet Carved Gaps and Dust Rings
Felipe Alarcón,Richard Teague,Richard Teague,Ke Zhang,Ke Zhang,Edwin A. Bergin,Marcelo Barraza-Alfaro +6 more
TL;DR: In this paper, the authors use a thermochemical code to focus on the chemical evolution that is occurring within the gas-depleted gap and the dust-rich ring often observed behind it, showing that the dust temperature at the midplane of the gap increases, enough to produce local sublimation of key volatiles and pushing the molecular layer closer to the mid plane, while it decreases in the dustrich ring, causing a higher volatile deposition onto the dust grain surfaces.