The Distribution of Giant Exoplanets over True and Projective Masses: Accounting for Observational Selection
- Авторы: Ananyeva V.I.1, Tavrov A.V.1,2, Venkstern A.A.1, Churbanov D.V.1,2, Shashkova I.A.1, Korablev O.I.1, Bertaux J.1,3
-
Учреждения:
- Space Research Institute
- Moscow Institute of Physics and Technology
- LATMOS-IPSL
- Выпуск: Том 53, № 2 (2019)
- Страницы: 124-137
- Раздел: Article
- URL: https://journal-vniispk.ru/0038-0946/article/view/171294
- DOI: https://doi.org/10.1134/S0038094619010027
- ID: 171294
Цитировать
Аннотация
To build the mass distribution of exoplanets discovered with the method of measuring the radial velocities, it is necessary to take into consideration the observational selection factors. We propose the detectability-window method to form homogeneous series of exoplanets. In addition, the errors in determining the masses are taken into account. The mass distributions of the transiting planets and the planets discovered with the radial-velocity method are compared in a range of 0.5 to 13 Jupiter masses.
Об авторах
V. Ananyeva
Space Research Institute
Автор, ответственный за переписку.
Email: lada@rssi.ru
Россия, Moscow, 117997
A. Tavrov
Space Research Institute; Moscow Institute of Physics and Technology
Email: lada@rssi.ru
Россия, Moscow, 117997; Dolgoprudnii, Moscow oblast, 141701
A. Venkstern
Space Research Institute
Email: lada@rssi.ru
Россия, Moscow, 117997
D. Churbanov
Space Research Institute; Moscow Institute of Physics and Technology
Email: lada@rssi.ru
Россия, Moscow, 117997; Dolgoprudnii, Moscow oblast, 141701
I. Shashkova
Space Research Institute
Email: lada@rssi.ru
Россия, Moscow, 117997
O. Korablev
Space Research Institute
Email: lada@rssi.ru
Россия, Moscow, 117997
J.-L. Bertaux
Space Research Institute; LATMOS-IPSL
Email: lada@rssi.ru
Россия, Moscow, 117997; Guyancourt, 78280
Дополнительные файлы
