Browsing by Author "Mirabel, I. F."

Now showing items 1-5 of 5

    • Are the hosts of gamma-ray bursts sub-luminous and blue galaxies? 
      Le Floc’h, E.; Duc, P.-A; Mirabel, I. F.; Sanders, D. B.; Bosch, G.; Diaz, R. J.; Donzelli, C. J.; Rodrigues, I.; Courvoisier, T. J. L.; Greiner, J.; Mereghetti, S.; Melnick, J.; Maza Sancho, José; Minniti, D. (EDP Sciences, 2003-03)
      We present K-band imaging observations of ten gamma-ray burst (GRB) host galaxies for which an optical and/or radio afterglow associated with the GRB event was clearly identified. Data were obtained with the Very Large ...
    • Large proper motions in the remarkable triple radio source in Serpens 
      Rodríguez, L. F.; Curiel, S.; Moran, J. M.; Mirabel, I. F.; Roth, M.; Garay Brignardello, Guido (UNIV CHICAGO PRESS, 1989-11-15)
      The triple radio source in the Serpens star formation region consists of a central object and two lobes with spectral indices characteristic of nonthermal emission. Measurements made at the Arecibo Observatory and the VLA ...
    • New evidence on the origin of the microquasar GRO J1655-40 
      Combi, J. A.; Bronfman Aguiló, Leonardo; Mirabel, I. F. (EDP SCIENCES S A, 2007-05)
      Aims. Motivated by the new determination of the distance to the microquasar GRO J1655- 40 by Foellmi et al. ( 2006, A&A, 457, 249), we conduct a detailed study of the distribution of the atomic ( HI) gas, molecular ( CO) ...
    • Southern ultraluminous infrared galaxies: An optical and infrared database 
      Duc, P. A.; Mirabel, I. F.; Maza Sancho, José (1997)
      We have carried out an optical and infrared study of 24 ultraluminous infrared galaxies in the southern hemisphere (SULIRGs). This flux limited, complete sample, has been extracted from the redshift survey of IRAS ...
    • VISTA Variables in the Via Lactea (VVV): The public ESO near-IR variability survey of the Milky Way 
      Minniti, D.; Lucas, P. W.; Emerson, J. P.; Saito, R. K.; Hempel Leyton, Marie Claire; Pietrukowicz, P.; Ahumada, A. V.; Alonso, M. V.; Alonso-García, J.; Arias, José I.; Bandyopadhyay, R. M.; Barbá, R. H.; Barbuy, B.; Bedin, Luigi R.; Bica, E.; Borissova, J.; Bronfman Aguiló, Leonardo; Carraro, Giovanni; Catelan, M.; Clariá, J. J.; Cross, N.; Grijs, R. de; Dékány, I.; Drew, J. E.; Fariña, C.; Feinstein, C.; Fernández Lajús, E.; Gamen, R. C.; Geisle, D.; Gieren, W.; Goldman, B.; Gonzalez, O. A.; Gunthardt, G.; Gurovich, S.; Hambly, N. C.; Irwin, M. J.; Ivanov, V. D.; Jordán, A.; Kerins, E.; Kinemuchi, K.; Kurtev, R.; López Corredoira, M.; Maccarone, Thomas J.; Masetti, N.; Merlo, D.; Messineo, M.; Mirabel, I. F.; Monaco, L.; Morelli, L.; Padilla, N.; Palma, T.; Parisi, M. C.; Pignata Libralato, Giuliano; Rejkuba, M.; Roman-Lopes, A.; Sale, S. E.; Schreiber, M. R.; Schröder, A. C.; Smith, M.; Sodré Jr., L.; Soto, M.; Tamura, M.; Tappert, C.; Thompson, M. A.; Toledo, I.; Zoccali, M. (2009-12-11)
      We describe the public ESO near-IR variability survey (VVV) scanning the Milky Way bulge and an adjacent section of the mid-plane where star formation activity is high. The survey will take 1929 hours of observations with ...