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Mostrando ítems 2081-2090 de 2112
Discovering exoplanets: hot jupiters [Frontiers and controversies in Astrophysics]
(Yale University, Open Yale Courses, 2011)
Conos concentradores de radiación para astronomía en longitudes de onda milimétricas
(Instituto Nacional de Astrofísica, Óptica y Electrónica, 2012)
Espectroscopia de Estrelas Be nos aglomerados NGC 4755 e NGC 6530
(UNIVERSIDADE ESTADUAL DE PONTA GROSSABRFisicaPrograma de Pós-Graduação em CiênciasUEPG, 2017)
Improving our ability to distinguish gravitational-wave signals from detector transient noise for the fourth LIGO-Virgo-KAGRA observing run
(Universidad de los AndesFísicaFacultad de CienciasDepartamento de Física, 2023-07-12)
A pesar de haber alcanzado sensibilidades capaces de detectar la amplitud extremadamente pequeña de las ondas gravitacionales (GWs), los datos de los detectores LIGO y Virgo contienen frecuentes ráfagas de ruido transitorio ...
VVV DR1: The first data release of the Milky Way bulge and southern plane from the near-infrared ESO public survey VISTA variables in the Vía Láctea
(Edp Sciences, 2012-01)
Context. The ESO public survey VISTA variables in the Vía Láctea (VVV) started in 2010. VVV targets 562 sq. deg in the Galactic bulge and an adjacent plane region and is expected to run for about five years. Aims. We ...
A ring system detected around the Centaur (10199) Chariklo
(Nature Publishing Group, 2014-04)
Hitherto, rings have been found exclusively around the four giant planets in the Solar System. Rings are natural laboratories in which to study dynamical processes analogous to those that take place during the formation ...
Benchmark stars for Gaia Fundamental properties of the Population II star HD 140283 from interferometric, spectroscopic, and photometric data
(EDP Sciences, 2015)
Metal-poor halo stars are important astrophysical laboratories that allow us to unravel details about many aspects of astrophysics, including the chemical conditions at the formation of our Galaxy, understanding the processes ...