Studying the resolved stellar populations of the different structural components that build massive galaxies directly unveils their assembly history. We aim at...
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PublicaciónA Duality in the Origin of Bulges and Spheroidal Galaxies
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PublicaciónA Perspective on the Milky Way Bulge Bar as Seen from the Neutron-capture Elements Cerium and Neodymium with APOGEE
This study probes the chemical abundances of the neutron-capture elements cerium and neodymium in the inner Milky Way from an analysis of a sample of ∼2000...
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PublicaciónBASS. XXXV. The M <SUB>BH</SUB>-σ* Relation of 105 Month Swift-BAT Type 1 AGNs
We present two independent measurements of stellar velocity dispersions (σ ⋆) from the Ca II H+K λ3969, 3934 and Mg I b λ 5183, 5172, 5167 region (3880-5550 Å)...
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NoticiaDescifran el enigma del agujero negro fugitivo
Un estudio, realizado por un equipo de investigación del Instituto de Astrofísica de Canarias (IAC), revela que una inusual y delgada estructura de estrellas...
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PublicaciónExploring the Stellar Age Distribution of the Milky Way Bulge Using APOGEE
We present stellar age distributions of the Milky Way bulge region using ages for ∼6000 high-luminosity ( $\mathrm{log}(g)\lt 2.0$ ), metal-rich ([Fe/H] ≥ -0.5)...
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PublicaciónFrom Naked Spheroids to Disky Galaxies: How Do Massive Disk Galaxies Shape Their Morphology?
We investigate the assembly history of massive disk galaxies and describe how they shape their morphology through cosmic time. Using SHARDS and HST data, we...