Probing the circumnuclear stellar populations of starburst galaxies in the near-infrared

2014/06/24 by N. Z. Dametto, R. Riffel, Rogério Riffel +6 · 2 citations
Physics and Astronomy · #Astronomy #Astronomy and Astrophysical Research #Astrophysics #Disc galaxy #Galaxies: Formation, Evolution, Phenomena #Galaxy #Infrared #Luminous infrared galaxy #Physics #Stellar, planetary, and galactic studies #astro-ph.GA

paper · pdf · doi:10.1093/mnras/stu1243

arxiv created 2014/06/24 · arxiv updated 2014/06/25 · openalex publication_date 2014/07/25 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

Accepted. Received, in original form We employ the NASA Infrared Telescope Facility’s near-infrared spectrograph SpeX at 0.8-2.4µm to investigate the spatial distribution of the stellar populations (SPs) in four well known

Citations

• Extreme Gas Kinematics in thez = 2.2 Powerful Radio Galaxy MRC 1138−262: Evidence for Efficient Active Galactic Nucleus Feedback in the Early Universe?
• Spextool: A Spectral Extraction Package for SpeX, a 0.8–5.5 Micron Cross‐Dispersed Spectrograph
• SpeX: A Medium‐Resolution 0.8–5.5 Micron Spectrograph and Imager for the NASA Infrared Telescope Facility
• A Method of Correcting Near‐Infrared Spectra for Telluric Absorption1
• Modelling the Spectral Energy Distribution of compact luminous infrared galaxies: Constraints from high frequency radio data
• STAR FORMATION IN GALAXIES ALONG THE HUBBLE SEQUENCE
• A probabilistic formulation for empirical population synthesis: sampling methods and tests
• The star formation histories of galaxies in the Sloan Digital Sky Survey

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