RAS PhysicsАстрономический журнал Astronomy Reports

  • ISSN (Print) 0004-6299
  • ISSN (Online) 3034-5170

MODELING OF TRANSIT ABSORPTIONS OF WARM NEPTUNE WASP-69b IN THE METASTABLE HELIUM LINE

PII
S30345170S0004629925030052-1
DOI
10.7868/S3034517025030052
Publication type
Article
Status
Published
Authors
Volume/ Edition
Volume 102 / Issue number 3
Pages
197-204
Abstract
This work presents the results of complex numerical modeling of the transit absorptions of the hot exoplanet WASP-69b in the metastable helium HeI(2S) line. The modeling was provided using a 3D MHD code, which allows for the simulation of effects that influence the absorption profile in various spectral lines and predicts a realistic distribution of the density of the main components and the structure of the interacting flows of planetary and stellar material. It was shown that the simulated transit absorption profiles closely match the height and width of the measured transit profiles, which allowed for the estimation of the physicochemical parameters in the area of exoplanet WASP-69b.
Keywords
гидродинамика спектральная линия профили плазма перенос излучения техника спектроскопия
Date of publication
14.10.2024
Year of publication
2024
Number of purchasers
0
Views
45

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