Browsing by Author "Casassus, S."

Now showing 1 - 11 of 11
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    Accretion kinematics through the warped transition disk in HD 142527 from resolved CO(6-5) observations
    (2015) Casassus, S.; Marino, S.; Perez, S.; Roman, P.; Dunhill, Alexander Charles; Armitage, P.; Cuadra Stipetich, Jorge Rodrigo; Wootten, A.; Van Der Plas, G.; Cieza, L.; Moral, V.; Christiaens, V.; Montesinos, M.
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    Characterization of low-mass companion HD 142527 B
    (2018) Christiaens, V.; Casassus, S.; Absil, O.; Kimeswenger, S.; Gonzalez, C. A. Gomez; Girard, J.; Ramirez, R.; Wertz, O.; Zurlo, A.; Wahhaj, Z.; Flores, C.; Salinas, V.; Jordán Colzani, Andrés Cristóbal; Mawet, D.
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    Criteria chilean clinical supervisors consider relevant when supervising : a qualitative study
    (2017) Araya, C.; Casassus, S.; Guerra Vio, Cristóbal; Salvo, D.; Zapata, J.; Krause Jacob, Mariane
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    Flows of gas through a protoplanetary gap
    (2013) Casassus, S.; Jordán Colzani, Andrés Cristóbal
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    HD 169142 in the eyes of ZIMPOL/SPHERE
    (2018) Bertrang, G.H.M.; Avenhaus, H.; Casassus, S.; Montesinos Armijo, Matías Alfredo; Kirchschlager, F.; Perez, S.; Cieza, L.; Wolf, S.
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    Is there really a debris disc around ζ2 reticuli?
    (2018) Faramaz, V.; Bryden, G.; Stapelfeldt, K.R.; Booth, M.; Bayo, A.; Beust, H.; Casassus, S.; Cuadra Stipetich, Jorge Rodrigo; Hales, A.; Hughes, A.M.; Olofsson, J.; Su, K.Y. L.; Wilner, D.J.
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    Planet formation signposts : Observability of circumplanetary disks via gas kinematics
    (2015) Pérez, Sebastián; Dunhill, Alexander Charles; Casassus, S.; Roman, P; Szulágyi, J.; Flores, C.; Marino, S.; Montesinos, M.
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    Separating extended disc features from the protoplanet in PDS 70 using VLT/SINFONI
    (2019) Christiaens, V.; Casassus, S.; Absil, O.; Cantalloube, F.; González, C. G.; Girard, J.; Ramírez, R.; Pairet, B.; Salinas, V.; Jordán Colzani, Andrés Cristóbal; Price, D. J.; Pinte, C.; Quanz, S. P.; Mawet, D.; Wahhaj, Z.
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    The dynamically disrupted gap in HD 142527
    (2012) Casassus, S.; Jordán Colzani, Andrés Cristóbal; Cuadra, Jorge
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    The State-of-Play of Anomalous Microwave Emission (AME) research
    (2018) Dickinson, Clive; Ali-Haimoud, Y.; Barr, A.; Battistelli, E. S.; Bell, A.; Bernstein, L.; Casassus, S.; Cleary, K.; Draine, B. T.; Genova-Santos, R.; Harper, S. E.; Hensley, B.; Hill-Valler, J.; Thiem Hoang; Israel, F. P.; Jew, L.; Lazaria
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    VISTA Milky Way Public Survey
    (2009) Minniti, D.; Lucas, P.; Ahumada, A. V.; Zoccali, M.; Catelan, Marcio; Morelli, L.; Tappert, C.; Pignata, G.; Toledo, I.; Ruiz, M. T.; Carraro, G.; Casassus, S.; Bronfman, L.; Barbá, R. H.; Gamen, R.; Gieren, W.; Geisler, D.; Pietrzynski, G.; Mennickent, R. E.; Kurtev, R.; Borissova, J.; Mirabel, F.; Ivanov, V. D.; Saviane, I.; Vanzi, L.; Monaco, L.; Rejkuba, M.; Messineo, M.; Bedin, L.; Stephens, A.; Barbuy, B.; Bica, E.; Clariá, J. J.; CASU (VDFS) Team; WFAU (VDFS) Team; Emerson, J.; Drew, J.; López-Correidora, M.; Martin, E.; Goldman, B.; Gianinni, T.; Eisloeffel, J.; Groot, P.; Fabregat, J.; Hambly, N.; Longmore, A.; Walton, N.; de Grijs, R.; Hoare, M.; Schroeder, A.; Naylor, T.; Barlow, M.; Zijlstra, A.; White, G.; Gosling, A.; McGowan, K.; Adamson, A.; Bandyopadhyay, R.; Thompson, M.; Cropper, M.; Lucey, J.; Kerins, E.; Hodgkin, S.; Pinfield, D.
    We propose a public IR variability survey, named ``Vista Variables in the Vía Láctea'' (VVV), of the Milky Way bulge and an adjacent section of the mid-plane where star formation activity is high. This would take 1920 hours, covering ∼ 10^9 point sources within an area of 520 sq deg, including 33 known globular clusters and ∼ 350 open clusters. The final products will be a deep IR atlas in 5 passbands and a catalogue of ∼ 10^6 variable point sources. These will produce a 3-D map of the surveyed region (unlike single-epoch surveys that only give 2-D maps) using well-understood primary distance indicators such as RR Lyrae stars. It will yield important information on the ages of the populations. The observations will be combined with data from MACHO, OGLE, EROS, VST, SPITZER, HST, CHANDRA, INTEGRAL, and ALMA for a complete understanding of the variable sources in the inner Milky Way. Several important implications for the history of the Milky Way, for globular cluster evolution, for the population census of the bulge and center, and for pulsation theory would follow from this survey....