Now showing items 20336-20355 of 20505

    • Sucapuca Pacara, Leslie Elizabeth (Universidad de Chile, 2017)
      Diversos modelos geoestadísticos permiten simular tipos de roca o, más generalmente, unidades geológicas en los yacimientos, entre los cuales se cuenta el modelo de simulación plurigaussiana y el de simulación secuencial ...
    • Gómez, Y.; Rodríguez, L. F.; Girart, J.M.; Garay Brignardello, Guido; Martí, J. (The American Astronomical Society, 2003-11-01)
      We present high angular resolution Very Large Array (VLA) and Berkeley-Illinois-Maryland Association (BIMA) observations of NH3, HCO+, HCN, and SO molecular emission and 1.4, 3.5, and 7 mm continuum emission toward the ...
    • Garay Brignardello, Guido; Gómez, Yolanda; Lizano, Susana; Brown, Robert L. (1998-07-10)
      We present high angular resolution VLA observations of the C92a, C110a, and C166a radio recombination lines of carbon from the region of massive star formation known as S88B. The observations reveal that the carbon ...
    • Torres, Rosa M.; Loinard, Laurent; Mioduszewski, Amy J.; Boden, Andrew F.; Franco Hernández, Ramiro; Vlemmings, Wouter H. T.; Rodríguez, Luis F. (2012-01-01)
      We present multi-epoch Very Long Baseline Array (VLBA) observations of V773 Tau A, the 51 day binary subsystem in the multiple young stellar system V773 Tau. Combined with previous interferometric and radial velocity ...
    • Espíritu, José; Peimbert, Antonio; Delgado-Inglada, Gloria; Ruiz, Mara (Universidad Nacional Autonoma de Mexico, 2017)
      We present a long-slit spectroscopic analysis of Herbig-Haro 202 and the surrounding gas of the Orion Nebula using data from the Very Large Telescope3. We determined the spatial variation of its physical conditions and ...
    • Campusano, Luis E.; Pelló, R.; Kneib, J. P.; Le Borgne, J. F.; Fort, B.; Ellis, R.; Mellier, Y.; Smail, I. (2001-11)
      We present the first results of a spectroscopic survey of faint lensed galaxies in the core of the galaxy cluster AC114 (z = 0.312) obtained from observations with the FORS1 spectrograph mounted on the VLT-Antu (Unit ...
    • Alves Brito, A.; Barbuy, B.; Zoccali, Manuela; Minniti, D.; Ortolani, S.; Hill, V.; Renzini, A.; Pasquini, L.; Bica, E.; Rich, R. M.; Meléndez, J.; Momany, Y. (EDP SCIENCES S A, 2006-12)
      Context. Metal-rich globular clusters trace the formation of bulges. Abundance ratios in the metal-rich globular clusters such as NGC 6553 can constrain the formation timescale of the Galactic bulge. Aims. The purpose of ...
    • Reggiani, M.; Meyer, M.; Chauvin, G.; Vigan, A.; Quanz, S.; Biller, B.; Bonavita, M.; Desidera, S.; Delorme, P.; Hagelberg, J.; Maire, Anne-Lise; Boccaletti, A.; Beuzit, J.; Buenzli, E.; Carson, J.; Covino, E.; Feldt, M.; Girard, J.; Gratton, R.; Henning, Thomas; Kasper, M.; Lagrange, A.; Mesa, D.; Messina, S.; Montagnier, G.; Mordasini, C.; Mouillet, D.; Schlieder, J.; Segransan, D.; Thalmann, C.; Zurlo, A. (EDP SCIENCES, 2016)
      Context. In recent years there have been many attempts to characterize the occurrence and distribution of stellar, brown dwarf (BD), and planetary-mass companions to solar-type stars with the aim of constraining formation ...
    • Maire, A.-L.; Rodet, L.; Lazzoni, C.; Boccaletti, A.; Brandner, W.; Galicher, R.; Cantalloube, F.; Mesa, D.; Klahr, H.; Beust, H.; Chauvin, G.; Desidera, S.; Janson, M.; Keppler, M.; Olofsson, J.; Augereau, J. -C.; Daemgen, S.; Henning, Thomas; Thebault, P.; Bonnefoy, M.; Feldt, M.; Gratton, R.; Lagrange, Anne Marie; Langlois, M.; Meyer, M. R.; Vigan, A.; D'Orazi, V.; Hagelberg, J.; Coroller, H. Le; Ligi, R.; Rouan, D.; Samland, M.; Schmidt, T.; Udry, S.; Zurlo, A.; Abe, L.; Carle, M.; Delboulbe, A.; Feautrier, P.; Magnard, Y.; Maurel, D.; Moulin, T.; Pavlov, A.; Perret, D.; Petit, C.; Ramos, J. R.; Rigal, F.; Roux, A.; Weber, L. (EDP Sciences, 2018-08-07)
      Context. A low-mass brown dwarf has recently been imaged around HR 2562 (HD 50571), a star hosting a debris disk resolved in the far infrared. Interestingly, the companion location is compatible with an orbit coplanar with ...
    • Lombart, Maxime; Chauvin, Gael Epely; Rojo Rubke, Patricio; Lagadec, Eric; Delorme, Philippe; Beust, Herve; Bonnefoy, Mickael; Galicher, Raphael; Gratton, Raffaele; Mesa, Dino; Bonavita, Mariangela; Allard, France; Bayo, Alberto; Boccaletti, Anthony; Desidera, Silvano; Girard, Julien; Jenkins, James Stewart; Klahr, H.; Laibe, G.; Lagrange, Anne Marie; Lazzoni, C.; Marleau, Gabriel Dominique; Minniti, Dante; Mordasini, C. (EDP Science, 2020)
      Context. Dusty debris disks around pre- and main-sequence stars are potential signposts for the existence of planetesimals and exoplanets. Giant planet formation is therefore expected to play a key role in the evolution ...
    • Viikinkoski, M.; Kaasalainen, M.; Durech, J.; Carry, B.; Marsset, M.; Fusco, T.; Dumas, C.; Merline, W.; Yang, B.; Berthier, J.; Kervella, Pierre; Vernazza, P. (EDP Sciences, 2015)
      We use the recently released Atacama Large Millimeter Array (ALMA) and VLT/SPHERE science verification data, together with earlier adaptive-optics images, stellar occultation, and lightcurve data to model the 3D shape and ...
    • López Morales, Sebastián (EDP Sciences, 2015)
      We present a detailed analysis of three extremely strong, intervening damped Lyman-α systems (ESDLAs, with log N(H i) ≥ 21.7) observed towards quasars with the Ultraviolet and Visual Echelle Spectrograph on the Very Large ...
    • Vedova, G. Dalla; Millour, F.; Souza, A. Domiciano de; Petrov, R. G.; Faes, D. Moser; Carciofi, A. C.; Kervella, Pierre; Rivinius, T. (EDP Sciences, 2017-05)
      Context. The mechanism of disk formation around fast-rotating Be stars is not well understood. In particular, it is not clear which mechanisms operate, in addition to fast rotation, to produce the observed variable ejection ...
    • Anthonioz, F.; Ménard, Francois; Pinte, Christophe; Le Bouquin, J. B.; Benisty, Myriam; Thi, W. F.; Absil, Olivier; Duchêne, G.; Augereau, J. C.; Berger, J. P.; Casassus Montero, Simón; Duvert, G.; Lazare, B.; Malbet, F.; Millan Gabet, R.; Schreiber, M. R.; Traub, W.; Zins, G. (EDP Sciences, 2015)
      Context. The properties of the inner disks of bright Herbig AeBe stars have been studied with near-infrared (NIR) interferometry and high resolution spectroscopy. The continuum (dust) and a few molecular gas species have ...
    • Garreaud Salazar, René; Rutllant Costa, José; Muñoz Alvarado, Raúl; Rahn, David; Ramos, M.; Figueroa, D. (COPERNICUS GESELLSCHAFT MBH, 2011)
      The VAMOS Ocean-Cloud-Atmosphere-Land Study Regional Experiment (VOCALS-REx) was a major field experiment conducted in spring of 2008 off southern Peru and northern Chile, aimed at better understanding the coupled climate ...
    • Robidoux, Philippe; Pastén, Daniela; Levresse, Gilles; Díaz, Gloria; Paredes, Dante (MDPI, 2021)
      Potential flank eruptions at the presently active Villarrica, Southern Andes Volcanic Zone (33.3–46 S) require the drawing of a comprehensive scenario of eruptive style dynamics, which partially depends on the degassing ...
    • Bórquez Oliva, Diego Fernando (Universidad de Chile, 2019)
      Los factores que afectan los spreads de bonos corporativos han sido ampliamente estudiados. Modelos estructurales de riesgo de crédito predicen que mientras mayor volatilidad accionaria y deuda tenga una firma, mayor es ...
    • Soto Vásquez, Rodrigo Alejandro (Universidad de Chile, 2020)
      La presente tesis estudia los efectos que tiene la volatilidad global de la tasa de cambio,tasa de interés e inflación sobre el crecimiento y otras variables macroeconómicas. Se sigue la literatura al explorar como la ...
    • Godfrey, Linda; Álvarez Amado, Fernanda (MDPI, 2020)
      The Li-rich brine contained within the halite body of the Salar de Atacama is uncommon for two reasons: First, it has an exceptionally high Li concentration, even compared to other closed basins in the Li triangle of South ...
    • Van Eaton, Alexa R.; Amigo, Álvaro; Bertin, Daniel; Mastin, Larry G.; Giacosa, Raúl E.; González, Jerónimo; Valderrama, Óscar; Fontijn, Karen; Behnke, Sonja A. (Amer Geophysical Union, 2016)
      Soon after the onset of an eruption, model forecasts of ash dispersal are used to mitigate the hazards to aircraft, infrastructure, and communities downwind. However, it is a significant challenge to constrain the model ...