Esta sección ofrece el acceso a la base de datos de Publicaciones que recopila los artículos del IAC publicados en revistas científicas. Por favor, pulsa la flecha del menú para ver todas las opciones de búsqueda y de ordenación de resultados; autor, revista, año, etc..
Además ofrece acceso al repositorio de preprints del IAC: https://research.iac.es/preprints/l
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The cometary activity very far from the Sun: the case of C/2007 D1 (LINEAR) and other stories of cometsNot AvailableMazzotta Epifani, E. et al.
Fecha de publicación:
92010 -
The Chemical Evolution of the Monoceros Ring/Galactic Anticenter Stellar StructureThe origin of the Galactic Anticenter Stellar Structure (GASS) or "Monoceros Ring"—a low-latitude overdensity at the edge of the Galactic disk spanning at least the second and third Galactic quadrants—remains controversial. Models for the origin of GASS generally fall into scenarios where either it is a part (e.g., warp) of the Galactic disk or itChou, Mei-Yin et al.
Fecha de publicación:
92010 -
The Afterglows of Swift-era Gamma-ray Bursts. I. Comparing pre-Swift and Swift-era Long/Soft (Type II) GRB Optical AfterglowsWe have gathered optical photometry data from the literature on a large sample of Swift-era gamma-ray burst (GRB) afterglows including GRBs up to 2009 September, for a total of 76 GRBs, and present an additional three pre-Swift GRBs not included in an earlier sample. Furthermore, we publish 840 additional new photometry data points on a total of 42Kann, D. A. et al.
Fecha de publicación:
92010 -
The ACS LCID Project. III. The Star Formation History of the Cetus dSph Galaxy: A Post-reionization FossilWe use deep HST/ACS observations to calculate the star formation history (SFH) of the Cetus dwarf spheroidal (dSph) galaxy. Our photometry reaches below the oldest main-sequence turnoffs, which allows us to estimate the age and duration of the main episode of star formation in Cetus. This is well approximated by a single episode that peaked roughlyMonelli, M. et al.
Fecha de publicación:
92010 -
Superdense Massive Galaxies in the ESO Distant Cluster Survey (EDisCS)We find a significant number of massive and compact galaxies in clusters from the ESO Distant Clusters Survey (EDisCS) at 0.4 z 1. They have similar stellar masses, ages, sizes, and axial ratios to local z ~ 0.04 compact galaxies in WIde field Nearby Galaxy clusters Survey (WINGS) clusters, and to z = 1.4-2 massive and passive galaxies found inValentinuzzi, T. et al.
Fecha de publicación:
92010