Article, 2024

Constraining the formation history of the HAT-P-11 system using atmospheric abundances

ASTRONOMY & ASTROPHYSICS, ISSN 0004-6361, Volume 681, 10.1051/0004-6361/202346835

Contributors

Chatziastros, Lena (Corresponding author) [1] Bitsch, B. [1] Schneider, Aaron David [2] [3] [4]

Affiliations

  1. [1] Max Planck Inst Astron, Konigstuhl 17, D-69117 Heidelberg, Germany
    2. [NORA names: Germany; Europe, EU; OECD];
  2. [2] Katholieke Univ Leuven, Inst Astron, Celestijnenlaan 200D, B-3001 Leuven, Belgium
    3. [NORA names: Belgium; Europe, EU; OECD];
  3. [3] Kobenhavn Univ, Niels Bohr Inst, Blegdamsvej 17, DK-2100 Copenhagen, Denmark
    4. [NORA names: KU University of Copenhagen; University; Denmark; Europe, EU; Nordic; OECD];
  4. [4] Kobenhavn Univ, Niels Bohr Inst, Blegdamsvej 17, DK-2100 Copenhagen, Denmark
    5. [NORA names: KU University of Copenhagen; University; Denmark; Europe, EU; Nordic; OECD]

Abstract

Abstract not displayed. As this article is not marked as Open Access, it is unclear if we are allowed to show the abstract. Please use the link in the sidebar to view the data provider version of the article including abstract.

Keywords

planet-disk interactions, planets and satellites: atmospheres, planets and satellites: formation

Data Provider: Clarivate

LINKS
-

Matching Records in NORA

SUBJECTS
+

METRICS
+