Explore the words cloud of the UFOS project. It provides you a very rough idea of what is the project "UFOS" about.
The following table provides information about the project.
MAX-PLANCK-GESELLSCHAFT ZUR FORDERUNG DER WISSENSCHAFTEN EV
|Coordinator Country||Germany [DE]|
|Total cost||1˙618˙125 €|
|EC max contribution||1˙618˙125 € (100%)|
1. H2020-EU.1.1. (EXCELLENT SCIENCE - European Research Council (ERC))
|Duration (year-month-day)||from 2018-06-01 to 2023-05-31|
Take a look of project's partnership.
|1||MAX-PLANCK-GESELLSCHAFT ZUR FORDERUNG DER WISSENSCHAFTEN EV||DE (Munich)||coordinator||1˙618˙125.00|
With each newly detected exoplanet system, the planet formation theory is constantly gaining weight in the astrophysical research. The planets origin is a mystery which can only be solved by understanding the protoplanetary disks evolution. Recent disk observations by the new class of interferometer telescopes are challenging the existing theory of planet formation. They reveal astonishing detailed structures of spirals and rings in the dust emission which have never been seen before. Those structures are often claimed to be caused by embedded planets, which is difficult to explain with current models. This growing discrepancy between observation and theory forces us to realize: a novel disk modeling is essential to move on. Separate gas or dust evolution models have reached their limit and the gap between those has to be closed. With the UFOS project, I propose an unique and ambitious approach to unite gas and dust evolution models for protoplanetary disks. For the first time, a single global model will mutually link self-consistently: a) the transport of gaseous disk material, b) the radiative transfer, c) magnetic fields and their dissipation and d) the transport and growth of the solid material in form of dust grains. The development, performing and post-analysis of the models will initiate a new age for the planet formation research. The project results will achieve 1) unprecedented self-consistent precision to answer the question if those novel observed structures are caused by embedded planets or by the gas dynamics itself; 2) to find the locations of dust concentration and growth to unveil the birth places of planets and 3) to close the gap and finally unify self-consistent models of the disk evolution with the new class of observations. Only such advanced models combined with multi-wavelength observations, can show us the process of planet formation, and so explain the origin of the various of planets and exoplanets in our solar neighborhood and beyond.
|Data Management Plan||Open Research Data Pilot||2020-02-27 15:01:51|
Take a look to the deliverables list in detail: detailed list of UFOS deliverables.
|year||authors and title||journal||last update|
Anibal Sierra, Susana Lizano, Enrique MacÃas, Carlos Carrasco-GonzÃ¡lez, Mayra Osorio, Mario Flock
An Analytical Model of Radial Dust Trapping in Protoplanetary Disks
published pages: 7, ISSN: 1538-4357, DOI: 10.3847/1538-4357/ab1265
|The Astrophysical Journal 876/1||2020-01-30|
M. Villenave, M. Benisty, W. R. F. Dent, F. MÃ©nard, A. Garufi, C. Ginski, P. Pinilla, C. Pinte, J. P. Williams, J. de Boer, J.-I. Morino, M. Fukagawa, C. Dominik, M. Flock, T. Henning, A. JuhÃ¡sz, M. Keppler, G. Muro-Arena, J. Olofsson, L. M. PÃ©rez, G. van der Plas, A. Zurlo, M. Carle, P. Feautrier, A. Pavlov, J. Pragt, J. Ramos, J.-F. Sauvage, E. Stadler, L. Weber
Spatial segregation of dust grains in transition disks
published pages: A7, ISSN: 0004-6361, DOI: 10.1051/0004-6361/201834800
|Astronomy & Astrophysics 624||2020-01-30|
N. Scepi, G. Lesur, G. Dubus, M. Flock
Turbulent and wind-driven accretion in dwarf novae threaded by a large-scale magnetic field
published pages: A49, ISSN: 0004-6361, DOI: 10.1051/0004-6361/201833921
|Astronomy & Astrophysics 620||2020-01-30|
Florian Kirchschlager, Gesa H-M Bertrang, Mario Flock
Intrinsic polarization of elongated porous dust grains
published pages: 1211-1219, ISSN: 0035-8711, DOI: 10.1093/mnras/stz1763
|Monthly Notices of the Royal Astronomical Society 488/1||2020-01-30|
Mario Flock, Neal J. Turner, Gijs D. Mulders, Yasuhiro Hasegawa, Richard P. Nelson, Bertram Bitsch
Planet formation and migration near the silicate sublimation front in protoplanetary disks
published pages: A147, ISSN: 0004-6361, DOI: 10.1051/0004-6361/201935806
|Astronomy & Astrophysics 630||2020-01-30|
M. Keppler, R. Teague, J. Bae, M. Benisty, T. Henning, R. van Boekel, E. Chapillon, P. Pinilla, J. P. Williams, G. H.-M. Bertrang, S. Facchini, M. Flock, Ch. Ginski, A. Juhasz, H. Klahr, Y. Liu, A. MÃ¼ller, L. M. PÃ©rez, A. Pohl, G. Rosotti, M. Samland, D. Semenov
Highly structured disk around the planet host PDS 70 revealed by high-angular resolution observations with ALMA
published pages: A118, ISSN: 0004-6361, DOI: 10.1051/0004-6361/201935034
|Astronomy & Astrophysics 625||2020-01-30|
A. Mignone, M. Flock, B. Vaidya
A Particle Module for the PLUTO Code. III. Dust
published pages: 38, ISSN: 1538-4365, DOI: 10.3847/1538-4365/ab4356
|The Astrophysical Journal Supplement Series 244/2||2020-01-30|
Dylan L Kloster, M Flock
Observable scattered light features from inclined and non-inclined planets embedded in protoplanetary discs
published pages: , ISSN: 0035-8711, DOI: 10.1093/mnras/stz1649
|Monthly Notices of the Royal Astronomical Society||2020-01-30|
S. Ertel, D. Kamath, M. Hillen, H. van Winckel, J. Okumura, R. Manick, H. M. J. Boffin, J. Milli, G. H.-M. Bertrang, L. Guzman-Ramirez, J. Horner, J. P. Marshall, P. Scicluna, A. Vaz, E. Villaver, R. Wesson, S. Xu
Resolved Imaging of the AR Puppis Circumbinary Disk
published pages: 110, ISSN: 1538-3881, DOI: 10.3847/1538-3881/aafe04
|The Astronomical Journal 157/3||2020-01-30|
Takahiro Ueda, Mario Flock, Satoshi Okuzumi
Dust Pileup at the Dead-zone Inner Edge and Implications for the Disk Shadow
published pages: 10, ISSN: 1538-4357, DOI: 10.3847/1538-4357/aaf3a1
|The Astrophysical Journal 871/1||2020-01-30|
Lucas A Cieza, Dary RuÃz-RodrÃguez, Antonio Hales, Simon Casassus, Sebastian PÃ©rez, Camilo Gonzalez-Ruilova, Hector CÃ¡novas, Jonathan P Williams, Alice Zurlo, Megan Ansdell, Henning Avenhaus, Amelia Bayo, Gesa H-M Bertrang, Valentin Christiaens, William Dent, Gabriel Ferrero, Roberto Gamen, Johan Olofsson, Santiago Orcajo, Karla PeÃ±aÂ RamÃrez, David Principe, Matthias R Schreiber, Gerrit van
The Ophiuchus DIsc Survey Employing ALMA (ODISEA) â€“ I: project description and continuum images at 28 au resolution
published pages: 698-714, ISSN: 0035-8711, DOI: 10.1093/mnras/sty2653
|Monthly Notices of the Royal Astronomical Society 482/1||2020-01-30|
Enrique MacÃas, Catherine C. Espaillat, Mayra Osorio, Guillem Anglada, JosÃ© M. Torrelles, Carlos Carrasco-GonzÃ¡lez, Mario Flock, Hendrik Linz, Gesa H.-M. Bertrang, Thomas Henning, JosÃ© F. GÃ³mez, Nuria Calvet, William R. F. Dent
Characterization of Ring Substructures in the Protoplanetary Disk of HD 169142 from Multiwavelength Atacama Large Millimeter/submillimeter Array Observations
published pages: 159, ISSN: 1538-4357, DOI: 10.3847/1538-4357/ab31a2
|The Astrophysical Journal 881/2||2020-01-30|
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