Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › Research › peer-review
Observations of the exoplanet WASP-32 b with the Main Stellar Spectrograph at the 6-m BTA telescope have revealed the presence of a significant change in the intensity and the equivalent width of the Ha spectral line in the spectrum of the parent star of WASP-32 at the time of planet's transit. These observations are discussed in the context of the presence of a hydrogen shell at WASP-32 b filling the Roche lobe of the planet.
| Translated title of the contribution | Спектроскопическое прохождение экзопланеты WASP-32 b |
|---|---|
| Original language | English |
| Title of host publication | STARS: FROM COLLAPSE TO COLLAPSE |
| Editors | YY Balega, DO Kudryavtsev, Romanyuk, IA Yakunin |
| Publisher | Astronomical Society of the Pacific |
| Pages | 376-378 |
| Number of pages | 3 |
| ISBN (Print) | 978-1-58381-904-3 |
| State | Published - 2017 |
| Event | Conference on Stars: From Collapse to Collapse - Nizhny Arkhyz Duration: 2 Oct 2016 → 6 Oct 2016 |
| Name | Astronomical Society of the Pacific Conference Series |
|---|---|
| Publisher | ASTRONOMICAL SOC PACIFIC |
| Volume | 510 |
| Conference | Conference on Stars: From Collapse to Collapse |
|---|---|
| City | Nizhny Arkhyz |
| Period | 2/10/16 → 6/10/16 |
ID: 9365837