Tipo de publicación: Sin árbitro

  • Publicación
    The downplayed role of secular processes in the co-evolution of galaxies and black holes
    According to the current co-evolution picture, most present-day galaxies experienced at least one phase of vigorous black hole (BH) activity in the past, during...
  • Publicación
    The Duration of Starbursts in Eighteen Nearby Dwarf Starburst Galaxies
    The duration of a starburst is a fundamental parameter affecting the evolution of galaxies yet, to date, observational constraints on the durations of...
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    The dust activity of the "transition" cometary object P/2010 C1 (Scotti)
    We report on the cometary activity of the minor body P/2010 C1 (Scotti), an active Centaur observed at 5.51 AU. The long-term dynamical behavior of this target...
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    The Dwarf galaxy Abundances and Radial-velocities Team (DART) Large Programme - A Close Look at Nearby Galaxies
    We review the progress of ESO/WFI Imaging and VLT/FLAMES spectroscopy of large numbers of individual stars in nearby dwarf spheroidal galaxies by the Dwarf...
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    The Dwarf Galaxy Leo A: A Survivor From the Epoch of Reionization
    We present the results of a program to derive the complete star-formation history of the Local Group dwarf irregular galaxy Leo A (DDO 69). Leo A is a low...
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    The dwarf galaxy population of nearby galaxy clusters
    The Fornax, Virgo, Ursa Major and Perseus galaxy clusters all have very different characteristics, in terms of their density, mass, and large-scale environment...
  • Publicación
    The Dwarf Spheroidal Galaxies Around the Milky Way
    We review the progress of ESO/WFI Imaging and VLT/FLAMES spectroscopy of large numbers of individual stars in nearby dwarf spheroidal galaxies by the Dwarf...
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    The Dynamical Evolution of Planetary Nebulae After the Fast Wind
    In this paper we explore the dynamics of ionization bounded planetary nebulae after the termination of the fast stellar wind. When the stellar wind becomes...
  • Publicación
    The Dynamical Gas Evolution of Low-and Intermediate-Mass Stars: PN Formation
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