A new stellar library in the region of the CO index at 2.3 μm

2008/06/26 by E. Mármol-Queraltó, N. Cardiel, A. J. Cenarro +6 · 2 citations
Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysics #Biology #Computer science #Context (archaeology) #Galaxies: Formation, Evolution, Phenomena #Index (typography) #Optics #Physics #Stellar, planetary, and galactic studies #Wavelength #World Wide Web #astro-ph

paper · pdf · doi:10.1051/0004-6361:200810044

26 pages, 15 figures, accepted for publication in A&A. Typos in Eq. 9, 11 and 12 fixed

arxiv created 2008/06/26 · openalex publication_date 2008/07/17 · arxiv updated 2009/12/01 · openalex created_date 2022/10/03 · openalex updated_date 2026/08/05

Abstract

Context. The analysis of unresolved stellar populations demands evolutionary synthesis models with realistic physical ingredients and extended wavelength coverage.

Citations

• The First Detection of Near-Infrared CN Bands in Active Galactic Nuclei: Signature of Star Formation
• An Infrared Spectroscopic Study of Eight Galactic Globular Clusters
• Probing the Central Regions of Nearby Compact Elliptical Galaxies
• A Catalog of Parameters for Globular Clusters in the Milky Way
• Nuclear Stellar Populations in theInfrared Space ObservatoryAtlas of Bright Spiral Galaxies
• Medium-resolution Isaac Newton Telescope library of empirical spectra - II. The stellar atmospheric parameters
• Evolutionary tracks and isochrones for low- and intermediate-mass stars: From 0.15 to 7 M_\odot, and from Z=0.0004 to 0.03
• Stellar population of ellipticals in different environments: near-infrared spectroscopic observations

Cited by

• Comparison of stellar population model predictions using optical and infrared spectroscopy
• The Infrared Telescope Facility (IRTF) spectral library: