We present a comprehensive analysis of the evolution of the morphological and structural properties of a large sample of galaxies at z = 3-9 using early James...
PublicaciónCEERS Key Paper. III. The Diversity of Galaxy Structure and Morphology at z = 3-9 with JWST
PublicaciónColors and color gradients in bulges of galaxies
We have obtained surface photometry in U, B, R, and I for a complete optically selected sample of 45 early-type spiral galaxies, to investigate the colors and...
PublicaciónComposite Bulges. III. A Study of Nuclear Star Clusters in Nearby Spiral Galaxies
We present photometric and morphological analyses of nuclear star clusters (NSCs)-very dense, massive star clusters present in the central regions of most...
PublicaciónDynamical simulations of the interacting galaxies in the NGC 520/UGC 957 system
Numerical simulations of the interacting galaxies in the NGC 520/UGC 957 system are presented. Two sets of models were produced to investigate the postulated...
PublicaciónExtragalactic Magnetism with SOFIA (SALSA Legacy Program). V. First Results on the Magnetic Field Orientation of Galaxies
We present the analysis of the magnetic field (B-field) structure of galaxies measured with far-infrared (FIR) and radio (3 and 6 cm) polarimetric observations...
PublicaciónFlares, Warps, Truncations, and Satellite: The Ultra-thin Galaxy UGC 11859
The structure of the outskirts of galaxies provides valuable information about their past and evolution. Due to their projected orientation, edge-on isolated...
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...
PublicaciónFurther evidence of continuity between elliptical and disc galaxies
The behavior of the isophotes of the E galaxies in a new photometric sample of 33 early-type galaxies belonging to the Virgo cluster (Caon) is compared to that...
PublicaciónFurther evidence of continuity between elliptical and disk galaxies.