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Allona Vazan
Allona Vazan
Astrophysics Research Center (ARCO), Department of Natural Sciences, The Open University of Israel
在 openu.ac.il 的电子邮件经过验证 - 首页
标题
引用次数
引用次数
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A chemical survey of exoplanets with ARIEL
G Tinetti, P Drossart, P Eccleston, P Hartogh, A Heske, J Leconte, ...
Experimental astronomy 46, 135-209, 2018
4202018
Jupiter’s evolution with primordial composition gradients
A Vazan, R Helled, T Guillot
Astronomy & Astrophysics 610, L14, 2018
1072018
How cores grow by pebble accretion-I. Direct core growth
MG Brouwers, A Vazan, CW Ormel
Astronomy & Astrophysics 611, A65, 2018
882018
The evolution and internal structure of Jupiter and Saturn with compositional gradients
A Vazan, R Helled, M Podolak, A Kovetz
The Astrophysical Journal 829 (2), 118, 2016
852016
The effect of composition on the evolution of giant and intermediate-mass planets
A Vazan, A Kovetz, M Podolak, R Helled
Monthly Notices of the Royal Astronomical Society 434 (4), 3283-3292, 2013
822013
Planet formation theory in the era of ALMA and Kepler: from pebbles to exoplanets
J Drazkowska, B Bitsch, M Lambrechts, GD Mulders, D Harsono, A Vazan, ...
arXiv preprint arXiv:2203.09759, 2022
802022
Equatorial retrograde flow in WASP-43b elicited by deep wind jets?
L Carone, R Baeyens, P Mollière, P Barth, A Vazan, L Decin, P Sarkis, ...
Monthly Notices of the Royal Astronomical Society 496 (3), 3582-3614, 2020
762020
Convection and mixing in giant planet evolution
A Vazan, R Helled, A Kovetz, M Podolak
The Astrophysical Journal 803 (1), 32, 2015
692015
How planets grow by pebble accretion-III. Emergence of an interior composition gradient
CW Ormel, A Vazan, MG Brouwers
Astronomy & Astrophysics 647, A175, 2021
592021
Explaining the low luminosity of Uranus: a self-consistent thermal and structural evolution
A Vazan, R Helled
Astronomy & Astrophysics 633, A50, 2020
592020
Ariel: Enabling planetary science across light-years
G Tinetti, P Eccleston, C Haswell, PO Lagage, J Leconte, T Lüftinger, ...
arXiv preprint arXiv:2104.04824, 2021
532021
How planets grow by pebble accretion-II. Analytical calculations on the evolution of polluted envelopes
MG Brouwers, CW Ormel
Astronomy & Astrophysics 634, A15, 2020
522020
A new perspective on the interiors of ice-rich planets: ice–rock mixture instead of ice on top of rock
A Vazan, R Sari, R Kessel
The Astrophysical Journal 926 (2), 150, 2022
482022
ON the evolution and survival of protoplanets embedded in a protoplanetary disk
A Vazan, R Helled
The Astrophysical Journal 756 (1), 90, 2012
372012
Contribution of the core to the thermal evolution of sub-Neptunes
A Vazan, CW Ormel, L Noack, C Dominik
The Astrophysical Journal 869 (2), 163, 2018
322018
The contribution of the ARIEL space mission to the study of planetary formation
D Turrini, Y Miguel, T Zingales, A Piccialli, R Helled, A Vazan, F Oliva, ...
Experimental Astronomy 46, 45-65, 2018
282018
How planets grow by pebble accretion-IV. Envelope opacity trends from sedimenting dust and pebbles
MG Brouwers, CW Ormel, A Bonsor, A Vazan
Astronomy & Astrophysics 653, A103, 2021
252021
TW Hya: an old protoplanetary disc revived by its planet
S Nayakshin, T Tsukagoshi, C Hall, A Vazan, R Helled, J Humphries, ...
Monthly Notices of the Royal Astronomical Society 495 (1), 285-304, 2020
252020
Exploring the link between star and planet formation with Ariel
D Turrini, C Codella, C Danielski, D Fedele, S Fonte, A Garufi, ...
Experimental Astronomy, 1-54, 2021
242021
Magnesium oxide-water compounds at megabar pressure and implications on planetary interiors
S Pan, T Huang, A Vazan, Z Liang, C Liu, J Wang, CJ Pickard, HT Wang, ...
Nature Communications 14 (1), 1165, 2023
182023
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