Add to ORKGThe near-infrared spectral region is becoming\ud a very useful wavelength range to detect and\ud quantify the stellar population of galaxies.Resumo publicado no periódico: Revista Mexicana de Astronomía y Astrofísica. Serie de Conferencias, v. 44, p. 82, 2014
Context: Near-infrared (hereafter NIR) data may provide complementary information to the traditional...
We study the central (inner few hundred parsecs) stellar populations of four starburst galaxies (NGC...
The study of stellar populations in early-type galaxies in different environments is a powerful tool...
The near-infrared spectral region is becoming a very useful wavelength range to detect and quantify ...
We performed a near-infrared (NIR; ∼1.0 –2.4 μm) stellar population study in a sample of early-type ...
We performed a near-infrared (NIR; ∼1.0 –2.4 μm) stellar population study in a sample of early-type ...
Context. A new generation of spectral synthesis models has been developed in recent years, but there...
Context. A new generation of spectral synthesis models has been developed in recent years, but there...
We present unresolved single stellar population synthesis models in the near-infrared (NIR) range. T...
We present unresolved single stellar population synthesis models in the near-infrared (NIR) range. T...
We present unresolved single stellar population synthesis models in the near-infrared (NIR) range. T...
We present unresolved single stellar population synthesis models in the near-infrared (NIR) range. T...
Theoretical thesis.Bibliography: pages 85-96.1. Introduction -- 2. Observations and data reduction -...
We study the central (inner few hundred parsecs) stellar populations of four starburst galaxies (NGC...
We study the central (inner few hundred parsecs) stellar populations of four starburst galaxies (NGC...
Context: Near-infrared (hereafter NIR) data may provide complementary information to the traditional...
We study the central (inner few hundred parsecs) stellar populations of four starburst galaxies (NGC...
The study of stellar populations in early-type galaxies in different environments is a powerful tool...
The near-infrared spectral region is becoming a very useful wavelength range to detect and quantify ...
We performed a near-infrared (NIR; ∼1.0 –2.4 μm) stellar population study in a sample of early-type ...
We performed a near-infrared (NIR; ∼1.0 –2.4 μm) stellar population study in a sample of early-type ...
Context. A new generation of spectral synthesis models has been developed in recent years, but there...
Context. A new generation of spectral synthesis models has been developed in recent years, but there...
We present unresolved single stellar population synthesis models in the near-infrared (NIR) range. T...
We present unresolved single stellar population synthesis models in the near-infrared (NIR) range. T...
We present unresolved single stellar population synthesis models in the near-infrared (NIR) range. T...
We present unresolved single stellar population synthesis models in the near-infrared (NIR) range. T...
Theoretical thesis.Bibliography: pages 85-96.1. Introduction -- 2. Observations and data reduction -...
We study the central (inner few hundred parsecs) stellar populations of four starburst galaxies (NGC...
We study the central (inner few hundred parsecs) stellar populations of four starburst galaxies (NGC...
Context: Near-infrared (hereafter NIR) data may provide complementary information to the traditional...
We study the central (inner few hundred parsecs) stellar populations of four starburst galaxies (NGC...
The study of stellar populations in early-type galaxies in different environments is a powerful tool...