Zobrazeno 1 - 9
of 9
pro vyhledávání: '"Borsato, Nicholas W."'
Autor:
Das, Pradosh Barun, Zucker, Daniel B., De Silva, Gayandhi M., Borsato, Nicholas W., Mura-Guzmán, Aldo, Buder, Sven, Ness, Melissa, Nordlander, Thomas, Casey, Andrew R., Martell, Sarah L., Bland-Hawthorn, Joss, de Grijs, Richard, Freeman, Ken C., Kos, Janez, Stello, Dennis, Lewis, Geraint F., Hayden, Michael R., Sharma, Sanjib
Analysing stellar parameters and abundances from nearly one million Gaia DR3 Radial Velocity Spectrometer (RVS) spectra poses challenges due to the limited spectral coverage (restricted to the infrared Ca II triplet) and variable signal-to-noise rati
Externí odkaz:
http://arxiv.org/abs/2410.12272
Autor:
Prinoth, Bibiana, Hoeijmakers, H. Jens, Pelletier, Stefan, Kitzmann, Daniel, Morris, Brett M., Seifahrt, Andreas, Kasper, David, Korhonen, Heidi H., Burheim, Madeleine, Bean, Jacob L., Benneke, Björn, Borsato, Nicholas W., Brady, Madison, Grimm, Simon L., Luque, Rafael, Stürmer, Julian, Thorsbro, Brian
Publikováno v:
A&A 678, A182 (2023)
Ultra-hot Jupiters are tidally locked with their host stars dividing their atmospheres into a hot dayside and a colder nightside. As the planet moves through transit, different regions of the atmosphere rotate into view revealing different chemical r
Externí odkaz:
http://arxiv.org/abs/2308.04523
Autor:
Lee, Elspeth K. H., Prinoth, Bibiana, Kitzmann, Daniel, Tsai, Shang-Min, Hoeijmakers, Jens, Borsato, Nicholas W., Heng, Kevin
Publikováno v:
Monthly Notices of the Royal Astronomical Society, Volume 517, Issue 1, November 2022, Pages 240 256
The atmospheres of ultra hot Jupiters (UHJs) are prime targets for the detection of molecules and atoms at both low and high spectral resolution. We study the atmospheres of the UHJs WASP-121b and WASP-189b by performing 3D general circulation models
Externí odkaz:
http://arxiv.org/abs/2210.11986
Autor:
Kitzmann, Daniel, Hoeijmakers, Jens H., Grimm, Simon L., Borsato, Nicholas W., Lueber, Anna, Prinoth, Bibiana
Publikováno v:
A&A 669, A113 (2023)
The atmospheres of ultra-hot Jupiters are highly interesting and unique chemical laboratories. Due to the very high atmospheric temperatures, their chemical composition is dominated by atoms and ions instead of molecules, and the formation of aerosol
Externí odkaz:
http://arxiv.org/abs/2112.11380
Autor:
Prinoth, Bibiana, Hoeijmakers, H. Jens, Kitzmann, Daniel, Sandvik, Elin, Seidel, Julia V., Lendl, Monika, Borsato, Nicholas W., Thorsbro, Brian, Anderson, David R., Barrado, David, Kravchenko, Kateryna, Allart, Romain, Bourrier, Vincent, Cegla, Heather M., Ehrenreich, David, Fisher, Chloe, Lovis, Christophe, Guzmán-Mesa, Andrea, Grimm, Simon, Hooton, Matthew, Morris, Brett M., Oreshenko, Maria, Pino, Lorenzo, Heng, Kevin
The temperature of an atmosphere decreases with increasing altitude, unless a shortwave absorber exists that causes a temperature inversion. Ozone plays this role in the Earth`s atmosphere. In the atmospheres of highly irradiated exoplanets, shortwav
Externí odkaz:
http://arxiv.org/abs/2111.12732
Streams of stars from captured dwarf galaxies and dissolved globular clusters are identifiable through the similarity of their orbital parameters, a fact that remains true long after the streams have dispersed spatially. We calculate the integrals of
Externí odkaz:
http://arxiv.org/abs/1907.02527
Akademický článek
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Autor:
Lee, Elspeth K H, Prinoth, Bibiana, Kitzmann, Daniel, Tsai, Shang-Min, Hoeijmakers, Jens, Borsato, Nicholas W, Heng, Kevin
Publikováno v:
Monthly Notices of the Royal Astronomical Society; 11/30/2022, Vol. 517 Issue 1, p240-256, 17p
Akademický článek
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