Erratum: Deconstructing double-barred galaxies in 2D and 3D - I. Classical nature of the dominant bulges
de Lorenzo-Cáceres, A. et al.
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2020
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It also provides access to IAC Preprints Repository here: https://research.iac.es/preprints/
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EL PAPEL DE LOS ESTALLIDOS DE FORMACIÓN ESTELAR EN LA FORMACIÓN Y EVOLUCIÓN DE GALAXIASEl objetivo principal de esta tesis es estudiar la evolución de las galaxias formadoras de estrellas durante los últimos 7 Gyrs. Las galaxias formadoras de estrellas de alto desplazamiento al rojo (z>1) difieren de sus contrapartidas locales en varios aspectos clave. Sus regiones formadoras de estrellas son de un orden de magnitud más grandes yAlejandro Lumbreras Calle
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12020 -
EL PAPEL DE LOS ESTALLIDOS DE FORMACIÓN ESTELAR EN LA FORMACIÓN Y EVOLUCIÓN DE GALAXIASEl objetivo principal de esta tesis es estudiar la evolución de las galaxias formadoras de estrellas durante los últimos 7 Gyrs. Las galaxias formadoras de estrellas de alto desplazamiento al rojo (z>1) difieren de sus contrapartidas locales en varios aspectos clave. Sus regiones formadoras de estrellas son de un orden de magnitud más grandes yAlejandro Lumbreras Calle
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12020 -
Dynamical Structure of Small Bulges Reveals Their Early Formation in ΛCDM ParadigmThe Λ cold dark matter (ΛCDM) paradigm of galaxy formation predicts that dense spheroidal stellar structures invariably grow at early cosmic time. These primordial spheroids evolve toward a virialized dynamical status as they finally become today's elliptical galaxies and large bulges at the center of disk galaxies. However, observations revealCostantin, Luca et al.
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Discovery of Two Pulsating Extremely Low-mass Pre-white Dwarf Candidates in the TESS Eclipsing BinariesWe report the discovery of two new pulsating extremely low-mass pre-white dwarf (pre-ELMV) candidates in the Transiting Exoplanet Survey Satellite (TESS) eclipsing binaries, TIC 149160359 and TIC 416264037. Their light curves show a typical feature of EL CVn-type binaries. The light-curve modeling indicates that they are both detached systems withWang, Kun et al.
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Detection of Ionized Calcium in the Atmosphere of the Ultra-hot Jupiter KELT-9bWith a dayside temperature in excess of 4500 K, comparable to a mid-K-type star, KELT-9b is the hottest planet known. Its extreme temperature makes KELT-9b a particularly interesting test bed for investigating the nature and diversity of gas giant planets. We observed the transit of KELT-9b at high spectral resolution (R ∼ 94,600) with the CARMENESTurner, Jake D. et al.
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12020