- PII
- S30345170S0004629925080039-1
- DOI
- 10.7868/S3034517025080039
- Publication type
- Article
- Status
- Published
- Authors
- Volume/ Edition
- Volume 102 / Issue number 8
- Pages
- 671-682
- Abstract
- A high-precision algorithm for interpreting transit light curves in the model of an eclipsing classical binary star-exoplanet system has been improved for interpretation moving from the variables “eccentricity (e)–periastron longitude (ω)” to the eccentricity components ( e cos , sin ω e ω ). The possibilities of interpretation by eccentricity components have been studied. It has been shown that the dependence of the minimum's shape on e sin ω alone is clearly expressed for small values of e and weakens with increasing e. The linear correlation between the radius value, which is characteristic of any values of e, is shown.
- Keywords
- двойные системы с экзопланетой транзитные кривые блеска эксцентриситет долгота периастра параметры орбиты
- Date of publication
- 01.08.2025
- Year of publication
- 2025
- Number of purchasers
- 0
- Views
- 42
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