Publicaciones

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  • The Most Distant Compact Groups
    We present photometric and spectroscopic observations of the members of three previously cataloged compact group (CG) candidates at redshifts z > 0.3. These confirm spectroscopic redshifts compatible with being gravitationally bound structures at redshifts 0.3112, 0.3848, and 0.3643, respectively, and then they are the most distant CGs known with
    Gutiérrez, C. M.

    Fecha de publicación:

    8
    2011
    Número de citas
    1
  • The Nature of Galactic Bulges from SAURON Absorption Line Strength Maps
    We discuss SAURON absorption line strength maps of a sample of 24 early-type spirals, mostly Sa. From the Lick indices H$eta$, Mg b and Fe 5015 we derive SSP-ages and metallicities. By comparing the scaling relations of Mg b and H beta and central velocity dispersion with the same relation for the edge-on sample of Falcon-Barroso et al. (2002) we
    Peletier, Reynier F. et al.

    Fecha de publicación:

    8
    2007
    Número de citas
    4
  • The nature of proximate damped Lyman α systems
    We present high-resolution echelle spectra of seven proximate damped Lyman α (PDLA) systems. The relative velocity separation of each PDLA from the background quasar is Δ V 3000 km s-1. Combining our sample with a further nine PDLAs from the literature we compare the chemical properties of the proximate systems with a control sample of intervening
    Ellison, Sara L. et al.

    Fecha de publicación:

    8
    2010
    Número de citas
    71
  • The Nature of the Nuclear H2O Masers of NGC 1068: Reverberation and Evidence for a Rotating Disk Geometry
    We report new (1995) Very Large Array (VLA) observations and (1984-1999) Effelsberg 100 m monitoring observations of the 22 GHz H2O maser spectrum of the Seyfert 2 galaxy NGC 1068. The sensitive VLA observations provide a registration of the 22 GHz continuum emission and the location of the maser spots with an accuracy of ~5 mas. Within the
    Gallimore, J. F. et al.

    Fecha de publicación:

    8
    2001
    Número de citas
    109
  • The nature of the X-ray transient SAX J1711.6-3808
    SAX J1711.6-3808 is an X-ray transient in the Galactic bulge that was active from January through May of 2001 and whose maximum 1-200 keV luminosity was measured to be 5x 10-9 erg cm-2 s-1 which is less than ~ 25% of the Eddington limit, if placed at a distance equal to that of the galactic center. We study the X-ray data that were taken of this
    in't Zand, J. J. M. et al.

    Fecha de publicación:

    8
    2002
    Número de citas
    20
  • The neutron star transient XTE J1701-407 has returned to quiescence after a 3-year long outburst
    The neutron star low-mass X-ray binary and long thermonuclear burst source XTE J1701-407 (ATel #1618) has been active ever since its discovery in 2008 June (ATel #1569), displaying a typical 2-10 keV luminosity of ~5E36 erg/s (assuming a distance D=5.0 kpc; ATel #2814). However, routine monitoring of the Galactic bulge with the PCA aboard RXTE
    Degenaar, N. et al.

    Fecha de publicación:

    8
    2011
    Número de citas
    3