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Determination of the exoplanet HD 189733 b atmospheric structure based on the multicolor photometric transit observations obtained with the HST and at the Caucasian Mountain Observatory

descriptionPublicationkeyboard_double_arrow_right Article 27 Dec 2024Publisher:Special Astrophysical Observatory of the Russian Academy of SciencesJournal:Modern astronomy: from the Early Universe to exoplanets and black holes
Authors: E. Bekesov;

doi: 10.26119/vak2024.129

Determination of the exoplanet HD 189733 b atmospheric structure based on the multicolor photometric transit observations obtained with the HST and at the Caucasian Mountain Observatory

Abstract

The paper presents a study of the exoplanet HD 189733 b based on the multicolor photometric observations obtained by the Hubble Space Telescope as well as on the equipment of the Caucasian Mountain Observatory. It is shown that with all other parameters fixed, the radius of the planet obtained from the interpretation of the light curves varies, which may be a consequence of the presence of an extended Rayleigh atmosphere.

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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
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