| Texto completo | |
| Autor(es): |
Selhorst, Caius Lucius
;
Valio, Adriana
;
Nandy, D
;
Valio, A
;
Petit, P
Número total de Autores: 5
|
| Tipo de documento: | Artigo Científico |
| Fonte: | LIVING AROUND ACTIVE STARS; v. 12, n. S328, p. 3-pg., 2017-01-01. |
| Resumo | |
Here we simulate the shape of a planetary transit observed at radio wavelengths. The simulations use a light curve of the K4 star HAT-P-11 and its hot Jupiter companion as proxy. From the HAT-P-11 optical light curve, a prominent spot was identified (1.10 R-P and 0.6 I-C). On the radio regime, the limb brighting of 30% was simulated by a quadratic function, and the active region was assumed to have the same size of the optical spot. Considering that the planet size is 6.35% of the the stellar radius, for the quiet star regions the transit depth is smaller than 0.5%, however, this value can increase to similar to 2% when covering an active region with 5.0 times the quiet star brightness temperature. (AU) | |
| Processo FAPESP: | 14/10489-0 - Estudo das mudanças no campo magnético solar a partir de observações rádio |
| Beneficiário: | Caius Lucius Selhorst |
| Modalidade de apoio: | Auxílio à Pesquisa - Regular |