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Mostrando ítems 1-10 de 485
On the incidence of wise infrared excess among solar analog, twin, and sibling stars
(The American Astronomical Society, 2020)
A Young White Dwarf with an Infrared Excess
(IOP Publishing, 2015)
Using observations of Spitzer/IRAC, we report the serendipitous discovery of excess infrared emission from a single white dwarf PG 0010+280. At a temperature of 27,220 K and a cooling age of 16 Myr, it is the hottest and ...
La región central M83 /
(2008-05)
La galaxia espiral M83, una SBb a tan sólo 4,5 Mpc, posee el núcleo starburst más cercano.
En esta tesis se presenta un estudio multibanda, utilizando diversas técnicas de espectroscopía 2D-3D.
Infrared excesses in stars with and without planets
(Instituto Nacional de Astrofísica, Óptica y Electrónica, 2015)
Infrared excesses in stars with and without planets
(Instituto Nacional de Astrofísica, Óptica y Electrónica, 2015)
Búsqueda de Planemos en la Nube Oscura Lynds 1495
(2011-05)
En este trabajo se presenta una búsqueda de Planemos (Planetary Mass Objects) en la nube oscura L 1495 en el complejo molecular de Tauro. Se emplean observaciones en las bandas K(2.2 μm) y H(1.6 μm) obtenidas con la cámara ...
Infrared and Raman spectra of [Re(CN)5NO]3- complex isolated in KCl matrix
(Elsevier Science, 2014-11-05)
We report here the infrared and Raman spectra of [Re(CN)5NO]3- complex as guest diluted in the KCl crystal lattice. According to the chemical analysis, the anion concentration in the KCl host matrix is in excess of 2% (in ...
94 Ceti: a triple star with a planet and dust disc
(OXFORD UNIV PRESS, 2016)
94 Ceti is a triple star system with a circumprimary gas giant planet and far-infrared excess. Such excesses around main sequence stars are likely due to debris discs, and are considered as signposts of planetary systems ...
A colour-excess extinction map of the southern Galactic disc from the VVV and GLIMPSE surveys
(2019)
An improved high-resolution and deep A(Ks) foreground dust extinction map is presented for the Galactic disc area within 295 degrees less than or similar to l less than or similar to 350 degrees, -1.0 degrees less than or ...
Modeling the infrared excess of solar analogs
(Instituto Nacional de Astrofísica, Óptica y Electrónica, 2012)