Browsing by Author "XX644848"
Now showing items 41-60 of 102
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(Universidad de ChileCyberDocs, 2010)
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(Universidad de ChilePrograma Cybertesis, 2007)
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(Universidad de ChilePrograma Cybertesis, 2008)La región G34.43+0.24 es una nube molecular opaca en la emisión del Infrarrojo medio, la cual presenta una forma filamentaria. Tiene una extensión de ~10 pc y está ubicada a una distancia de 3.7 kpc. Esta región se escogió ...
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(Universidad de ChilePrograma Cybertesis, 2009)
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(2003-12-01)We present Very Long Baseline Array proper-motion measurements of water masers toward two young stellar objects (YSOs) of the W75 N star-forming region. We find that these two objects are remarkable for having a similar ...
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(Universidad de ChilePrograma Cybertesis, 2007)
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(The Korean Astronomical Society, 2015-09)The physical and chemical properties of prestellar cores, especially massive ones, are still far from being well understood due to the lack of a large sample. The low dust temperature (< 14 K) of Planck cold clumps makes ...
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(Universidad de Chile, 2011)El objetivo de esta tesis fue la de caracterizar las propiedades físicas de zonas de formación de estrellas masivas en nubes moleculares y que se encuentran localizadas en la Galaxia externa austral; y realizar una ...
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(2010-02-10)We report molecular line and dust continuum observations, made with the Swedish-ESO Submillimeter Telescope, toward four young high-mass star-forming regions associated with highly luminous (L > 6 × 105 L ) Infrared Astronomical ...
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(2010-02-10)We present sensitive near-infrared (J, H, and K) imaging observations toward four luminous massive star-forming regions in the Norma Spiral Arm: G324.201+0.119, G328.307+0.432, G329.337+0.147, and G330.949−0.174. We ...
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(OXFORD UNIV PRESS, 2016)Recent surveys of dust continuum emission at sub-mm wavelengths have shown that filamentary molecular clouds are ubiquitous along the Galactic plane. These structures are inhomogeneous, with overdensities that are sometimes ...
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(The American Astronomical Society, 2015-01-20)We report molecular line observations, made with ASTE and SEST, and dust continuum observations at 0.87 mm, made with APEX, toward the cold dust core G305.136+0.068. The molecular observations show that the core is isolated ...
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(EDP Sciences, 2016)Context. Ring-like structures in the interstellar medium (ISM) are commonly associated with high-mass stars. Kinematic studies of large structures in giant molecular clouds (GMCs) toward these ring-like structures may help ...
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(Universidad de ChilePrograma Cybertesis, 2007)
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(UNIV CHICAGO PRESS, 2007-11-10)We report observations of 6 cm, 3.6 cm, 1.3 cm, and 7 mm radio continuum, conducted with the Very Large Array, toward IRAS 18566+0408, one of the few sources known to harbor H(2)CO6 cm maser emission. Our observations ...
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(IOP PUBLISHING LTD, 2008-06)The triple radio source detected in association with the luminous infrared source IRAS 16547-4247 has previously been studied with high angular resolution and high sensitivity with the Very Large Array at 3.6 cm wavelength. ...
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(Oxford University Press, 2020)We present new Atacama Large Millimeter/submillimeter Array observations of the tadpole, a small globule in the Carina Nebula that hosts the HH 900 jet+outflow system. Our data include (CO)-C-12, (CO)-C-13, (CO)-O-18 J=2-1, ...
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(Oxford Univ Press, 2020)We combine Multi-Unit Spectroscopic Explorer and Atacama Large Millimeter/sub-millimeter Array observations with theoretical models to evaluate how a tadpole-shaped globule located in the Carina Nebula has been influenced ...
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Infall signatures in a prestellar core embedded in the high-mass 70 mu m Dark IRDC G331.372-00.116 (IOP Publishing, 2018-07)Using Galactic Plane surveys, we have selected a massive (1200M circle dot), cold (14 K) 3.6-70 mu m dark IRDC, G331.372-00.116. This infrared dark cloud (IRDC) has the potential to form high-mass stars, and given the ...
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(Universidad de Chile, 2012)Uno de los problemas claves en el estudio de la formación de estrellas es determinar si acaso el paradigma de formación de estrellas de baja masa, específicamente, contracción gravitacional y la posterior presencia de un ...
