Constraining the origin of giant exoplanets via elemental abundance measurements
Astronomy & Astrophysics, 2022 - aanda.org
The origin of close-in giant planets is a key open question in planet formation theory. The
two leading models are (i) formation at the outer disk followed by migration and (ii) in situ …
two leading models are (i) formation at the outer disk followed by migration and (ii) in situ …
Constraining the origin of giant exoplanets via elemental abundance measurements
H Knierim, S Shibata, R Helled - Astronomy and …, 2022 - ui.adsabs.harvard.edu
The origin of close-in giant planets is a key open question in planet formation theory. The
two leading models are (i) formation at the outer disk followed by migration and (ii) in situ …
two leading models are (i) formation at the outer disk followed by migration and (ii) in situ …
Constraining the origin of giant exoplanets via elemental abundance measurements
H Knierim, S Shibata, R Helled - Astronomy and Astrophysics, 2022 - zora.uzh.ch
The origin of close-in giant planets is a key open question in planet formation theory. The
two leading models are (i) formation at the outer disk followed by migration and (ii) in situ …
two leading models are (i) formation at the outer disk followed by migration and (ii) in situ …
Constraining the origin of giant exoplanets via elemental abundance measurements
H Knierim, S Shibata, R Helled - arXiv preprint arXiv:2209.01240, 2022 - arxiv.org
The origin of close-in giant planets is a key open question in planet formation theory. The
two leading models are (i) formation at the outer disk followed by migration and (ii) in situ …
two leading models are (i) formation at the outer disk followed by migration and (ii) in situ …
[PDF][PDF] Constraining the origin of giant exoplanets via elemental abundance measurements
H Knierim, S Shibata, R Helled - measurements, 2022 - scholar.archive.org
The origin of close-in giant planets is a key open question in planet formation theory. The
two leading models are (i) formation at the outer disk followed by migration and (ii) in situ …
two leading models are (i) formation at the outer disk followed by migration and (ii) in situ …
[PDF][PDF] Constraining the origin of giant exoplanets via elemental abundance measurements
H Knierim, S Shibata, R Helled - A&A, 2022 - scholar.archive.org
The origin of close-in giant planets is a key open question in planet formation theory. The
two leading models are (i) formation at the outer disk followed by migration and (ii) in situ …
two leading models are (i) formation at the outer disk followed by migration and (ii) in situ …
Constraining the origin of giant exoplanets via elemental abundance measurements
H Knierim, S Shibata, R Helled - Astronomy and …, 2022 - ui.adsabs.harvard.edu
The origin of close-in giant planets is a key open question in planet formation theory. The
two leading models are (i) formation at the outer disk followed by migration and (ii) in situ …
two leading models are (i) formation at the outer disk followed by migration and (ii) in situ …