Zobrazeno 1 - 10
of 1 984
pro vyhledávání: '"Star activity"'
Autor:
Ketzer, Laura, Poppenhaeger, Katja
The detected exoplanet population displays a dearth of planets with sizes of about two Earth radii, the so-called radius gap. This is interpreted as an evolutionary effect driven by a variety of possible atmospheric mass loss processes of exoplanets.
Externí odkaz:
http://arxiv.org/abs/2209.05860
Autor:
Araújo, Alexandre, Valio, Adriana
Stellar magnetic activity, just like that of the Sun, manifests itself in the form of flares and spots on the surface of the star. In the solar case, the largest flares originate from large active regions. In this work, we present a study of the acti
Externí odkaz:
http://arxiv.org/abs/2111.05452
Akademický článek
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Autor:
Poppenhaeger, K., Schmitt, J. H. M. M.
The activity levels of stars are influenced by several stellar properties, such as stellar rotation, spectral type and the presence of stellar companions. In analogy to binaries, planetary companions are also thought to be able to cause higher activi
Externí odkaz:
http://arxiv.org/abs/1106.0189
Autor:
Castillo, Ana F., Orlando, Ulises, Helfenberger, Katia E., Poderoso, Cecilia, Podesta, Ernesto J. *
Publikováno v:
In Molecular and Cellular Endocrinology 15 June 2015 408:73-79
Autor:
Miljkovic, Marija1, Malesevic, Milka1, Filipic, Brankica1,2, Vukotic, Goran1,3, Kojic, Milan1
Publikováno v:
BioMed Research International. 1/29/2018, Vol. 2018, p1-10. 10p.
Autor:
Ketzer, L1,2 (AUTHOR) ketzer.laura@gmail.com, Poppenhaeger, K1,2 (AUTHOR)
Publikováno v:
Monthly Notices of the Royal Astronomical Society. Jan2023, Vol. 518 Issue 2, p1683-1706. 24p.
Autor:
Alexandre Araújo, Adriana Valio
Stellar magnetic activity, just like that of the Sun, manifests itself in the form of flares and spots on the surface of the star. In the solar case, the largest flares originate from large active regions. In this work, we present a study of the acti
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ce656f97902e1eccecf4b9a2938e3991
Autor:
Souza, Alexandre Araújo de
Publikováno v:
Biblioteca Digital de Teses e Dissertações do Mackenzie
Universidade Presbiteriana Mackenzie (MACKENZIE)
instacron:MACKENZIE
Universidade Presbiteriana Mackenzie (MACKENZIE)
instacron:MACKENZIE
IPM - Instituto Presbiteriano Mackenzie MackPesquisa - Fundo Mackenzie de Pesquisa Estrelas do tipo solar podem apresentar intensa atividade magnética. Nesta tese, apresentamos um estudo sobre atividade estelar em sistemas planetários com estrelas
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______3056::79a2a84cfd5e80c01f51cef687c75d69
https://dspace.mackenzie.br/handle/10899/28851
https://dspace.mackenzie.br/handle/10899/28851