Repositorio Académico de la Universidad de Chile

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    - Repositorio Académico de la Universidad de Chile


Facultades e institutos

Recently Added

  • Acevedo Guerra, Jorge (Universidad de Chile, Facultad de Filosofía y Humanidades, 2003)
  • Martínez Gutiérrez, Juan Pablo (2014)
    Introducción: El color de los dientes puede ser mejorado por una serie de técnicas, una de las más populares en nuestros días es el blanqueamiento At-Home. La efectividad de este tipo de blanqueamiento es uno de los ...
  • Escala Astorquiza, Andrés; Randriamanakoto, Z.; Vaisanen, P.; Kankare, E.; Kotilainen, J.; Mattila, S.; Ryder, S. (The American Astronomical Society, 2013-10-01)
    We have established a relation between the brightest super star cluster (SSC) magnitude in a galaxy and the host star formation rate (SFR) for the first time in the near-infrared (NIR). The data come from a statistical ...
  • Hamuy Wackenhut, Mario; Anderson, J.; Taddia, F.; Stritzinger, M.; Sollerman, J.; Phillips, M.; Boldt, L.; Campillay, A.; Castellón, S.; Contreras, C.; Folatelli, G.; Heinrich-Josties, E.; Krzeminski, W.; Morrell, N.; Burns, C.; Freedman, W.; Madore, B.; Persson, S.; Suntzef, N. (EDP Sciences, 2013-04-10)
    Aims. The observational diversity displayed by various Type IIn supernovae (SNe IIn) is explored and quantified. In doing so, a more coherent picture ascribing the variety of observed SNe IIn types to particular progenitor ...
  • Hamuy Wackenhut, Mario; Phillips, M.; Simon, Joshua; Morrell, Nidia; Burns, Christopher; Cox, Nick; Foley, Ryan; Karakas, Amanda; Patat, F.; Sternberg, A.; Williams, R.; Gal-Yam, A.; Hsiao, E.; Leonard, D.; Persson, Sven; Stritzinger, Maximilian; Thompson, I.; Campillay, Abdo; Contreras, Carlos; Folatelli, Gaston; Freedman, Wendy; Roth, Miguel; Shields, Gregory; Suntzeff, Nicholas; Chomiuk, Laura; Ivans, Inese; Madore, Barry; Penprase, B.; Perley, Daniel; Pignata, G.; Preston, G.; Soderberg, Alicia (The American Astronomical Society, 2013-11-10)
    High-dispersion observations of the Na i D λλ5890, 5896 and K i λλ7665, 7699 interstellar lines, and the diffuse interstellar band at 5780 Å in the spectra of 32 Type Ia supernovae are used as an independent means of ...

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