Not Available
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
-
Age Dating a Starburst: Gemini/CIRPASS Observations of the Core of M 83Ryder, S. et al.122004
-
Age Estimates for Globular Clusters in NGC 1399
We present high signal-to-noise Keck spectra for 10 globular clusters associated with the giant Fornax elliptical galaxy NGC 1399 and compare measured line indices with current stellar population models. Our data convincingly demonstrate, for the first time, that at least some of the clusters in a giant elliptical galaxy have supersolar abundance
Forbes, Duncan A. et al.Fecha de publicación:
122001 -
AGN Activity and Circumnuclear Star Formation in Nearby Galaxies
We have selected a sample of nearby galaxies where an AGN (Seyfert or LINER) coexists with circumnuclear star formation. We use the highest spatial resolution data available now (HST UV, optical, and near-infrared [IR]; radio) and in the future (mid-IR with Spitzer and CanariCam) with spatial resolutions of 3-25 pc for our sample. The main goal of
Alonso-Herrero, A. et al.Fecha de publicación:
122005 -
AKARI and Spitzer Observations of Heavily Obscured C-rich AGB/Post-AGB Stars
We present AKARI/IRC and Spitzer/IRS observations of a selected sample of galactic IRAS sources considered to be heavily obscured AGB / post-AGB stars based on their characteristic IRAS colours. All of them are completely invisible in the optical range but extremely bright in the infrared. Based on AKARI and Spitzer spectroscopy and using DUSTY we
García-Hernández, D. A. et al.Fecha de publicación:
122009 -
AKARI/IRC Observations of Heavily Obscured Oxygen-Rich AGB and Post-AGB Stars
We present AKARI/IRC observations of a sample of six extremely red IRAS sources, of which three are variable OH/IR stars and the rest are early post-AGB stars. The OH/IR stars show a red continuum with the expected strong 10 μm silicate absorption feature, while the post-AGB stars show an even redder continuum accompanied with a comparably weak
Bunzel, F. et al.Fecha de publicación:
122009 -
Al Comae, Not So Red Afterall; Photometry and Spectroscopy of a Very Faint TOAD.
A red inter-loper has been detected in the vicinity of the faint Tremendous Outburst Amplitude Dwarf (TOAD) AL Comae, with a 3.95 arc-seconds separation between the center of both systems. New infrared photometry was taken with the 2.1m IRIM camera on the observation nights of July 11 and 12 of 1997. Analysis of this data shows that the previously
Galvan, F. J. et al.Fecha de publicación:
121999