Zobrazeno 1 - 4
of 4
pro vyhledávání: '"Pablo Mauas"'
Autor:
Girish M. Duvvuri, J. Sebastian Pineda, Zachory K. Berta-Thompson, Alexander Brown, Kevin France, Adam F. Kowalski, Seth Redfield, Dennis Tilipman, Mariela C. Vieytes, David J. Wilson, Allison Youngblood, Cynthia S. Froning, Jeffrey Linsky, R. O. Parke Loyd, Pablo Mauas, Yamila Miguel, Elisabeth R. Newton, Sarah Rugheimer, P. Christian Schneider
Publikováno v:
The Astrophysical Journal, 913(1)
Characterizing the atmospheres of planets orbiting M dwarfs requires understanding the spectral energy distributions of M dwarfs over planetary lifetimes. Surveys like MUSCLES, HAZMAT, and FUMES have collected multiwavelength spectra across the spect
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::69681fa4c8f8fb30d9029dda950021bf
Autor:
Jeffrey L. Linsky, Brian E. Wood, Allison Youngblood, Alexander Brown, Cynthia S. Froning, Kevin France, Andrea P. Buccino, Steven R. Cranmer, Pablo Mauas, Yamila Miguel, J. Sebastian Pineda, Sarah Rugheimer, Mariela Vieytes, Peter J. Wheatley, David J. Wilson
Publikováno v:
The Astrophysical Journal, 902(1), 3
Extreme-ultraviolet and X-ray emissions from stellar coronae drive mass loss from exoplanet atmospheres, and ultraviolet emission from stellar chromospheres drives photo-chemistry in exoplanet atmospheres. Comparisons of the spectral energy distribut
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9874d893023a4c7e226fff264d262dc6
https://ui.adsabs.harvard.edu/abs/2020ApJ...902....3L
https://ui.adsabs.harvard.edu/abs/2020ApJ...902....3L
Autor:
J. M. Fontenla, Jeffrey L. Linsky, Jesse Garrison, Kevin France, A. Buccino, Pablo Mauas, Mariela Vieytes, Lucianne M. Walkowicz
Publikováno v:
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Stellar radiation from X-rays to the visible provides the energy that controls the photochemistry and mass loss from exoplanet atmospheres. The important extreme ultraviolet (EUV) region (10--91.2~nm) is inaccessible and should be computed from a rel
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7c36ec8bd1e0b29277d8be88ff525afb
Autor:
Kevin France, Cynthia S. Froning, Jeffrey L. Linsky, Aki Roberge, John T. Stocke, Feng Tian, Rachel Bushinsky, Jean-Michel Désert, Pablo Mauas, Mariela Vieytes, Lucianne M. Walkowicz
The spectral and temporal behavior of exoplanet host stars is a critical input to models of the chemistry and evolution of planetary atmospheres. At present, little observational or theoretical basis exists for understanding the ultraviolet spectra o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::505ae9c1a1f844f0ee6e8ceec64087dc