
Universidad de Valparaíso
Articles
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Jan 13, 2025 |
noticias.uestatales.cl | Universidad de Valparaíso
Una sala psicosocial que será instalada en la escuela básica Tomás Vargas y Arcaya de Maipú, construida con el acero fundido de más de 24 mil armas incautadas en 2024, se encuentran diseñando en la Escuela de Arquitectura de la Universidad de Valparaíso.
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Nov 4, 2024 |
academic.oup.com | Facultad de Ciencias |Universidad de Valparaíso |Universidad de Concepcion |Puerto Madryn
In all areas where fishing activities overlap with feeding and/or breeding areas for pinnipeds (seals, sea lions, and walrus), there is a high probability of operational interactions (Harwood and Croxall 1988, Riedman 1990, Wickens 1995, Bjørge et al. 2002, Jackson et al. 2024).
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Aug 12, 2024 |
revistadesociologia.uchile.cl | Universidad de Valparaíso
Bringel,Breno (2017): “Movimientos sociales y la nueva geopolítica de la indignación global”, pgs 29-36. En Bringel, Breno y Pleyers, Geoffrey: Protesta e Indignación Global. CLACSO. Draper, Susana (2018) México 1968: experimentos de la libertad, constelaciones de la democracia. México: Siglo XXI. Sassen, Saskia (2007): Una sociología de la globalización.
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Aug 1, 2024 |
academic.oup.com | Instituto de Astrofísica |Santiago Chile |Facultad de Ciencias |Universidad de Valparaíso
NGC 6357, a star-forming complex at ∼1.7 kpc from the Sun, contains giant molecular clouds and three prominent star clusters alongside HII regions, very massive stars and thousands of young stellar objects in different evolutionary stages. We present a combined infrared kinematic and time domain study of the line of sight towards this region enabled by the VVVX survey. In terms of kinematics, a novel discovery emerges: an asymmetrical distribution in the vector point diagram.
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Aug 1, 2024 |
academic.oup.com | Instituto de Astrofísica |Facultad de Ciencias |Universidad de Valparaíso |Departamento de Ciencias
The study of different star-forming regions and their stellar populations, as well as the reconstruction of their star formation history and structure need astrometric and kinematic data with the lowest levels of uncertainty possible. Thanks to the Gaia satellite (Gaia Collaboration et al.
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