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Leo V (dwarf galaxy)

  • The Detailed Properties of Leo V, Pisces II and Canes Venatici II

    The Detailed Properties of Leo V, Pisces II and Canes Venatici II

  • The Feeble Giant. Discovery of a Large and Diffuse Milky Way Dwarf Galaxy in the Constellation of Crater

    The Feeble Giant. Discovery of a Large and Diffuse Milky Way Dwarf Galaxy in the Constellation of Crater

  • What Is an Ultra-Faint Galaxy?

    What Is an Ultra-Faint Galaxy?

  • Searching for Dark Matter Annihilation in Recently Discovered Milky Way Satellites with Fermi-Lat A

    Searching for Dark Matter Annihilation in Recently Discovered Milky Way Satellites with Fermi-Lat A

  • Dark Matter Dominated Objects Louie Strigari Stanford Milky Way Circa 2009

    Dark Matter Dominated Objects Louie Strigari Stanford Milky Way Circa 2009

  • Neutral Hydrogen in Local Group Dwarf Galaxies

    Neutral Hydrogen in Local Group Dwarf Galaxies

  • Draft181 182Chapter 10

    Draft181 182Chapter 10

  • Arxiv:1010.2231V2 [Astro-Ph.CO] 10 Nov 2011 Vnfrjs Rctie L 08 Ono Ta.20) Howe 2009)

    Arxiv:1010.2231V2 [Astro-Ph.CO] 10 Nov 2011 Vnfrjs Rctie L 08 Ono Ta.20) Howe 2009)

  • Arxiv:2101.00013V2 [Astro-Ph.GA] 3 Aug 2021

    Arxiv:2101.00013V2 [Astro-Ph.GA] 3 Aug 2021

  • Dwarf Cosmology with the Stromlo Missing Satellites Survey

    Dwarf Cosmology with the Stromlo Missing Satellites Survey

  • The Darkest Galaxies

    The Darkest Galaxies

  • On the Nature of the Stellar Bridge Between Leo IV and Leo V

    On the Nature of the Stellar Bridge Between Leo IV and Leo V

  • The First Tidally Disrupted Ultra-Faint Dwarf Galaxy?-Spectroscopic

    The First Tidally Disrupted Ultra-Faint Dwarf Galaxy?-Spectroscopic

  • Boötes-I, Segue 1, the Orphan Stream and CEMP-No Stars: Extreme Systems Quantifying Feedback and Chemical Evolution in the Oldest and Smallest Galaxies

    Boötes-I, Segue 1, the Orphan Stream and CEMP-No Stars: Extreme Systems Quantifying Feedback and Chemical Evolution in the Oldest and Smallest Galaxies

  • Dynamical Evidence for a Strong Tidal Interaction Between the Milky Way and Its Satellite, Leo V

    Dynamical Evidence for a Strong Tidal Interaction Between the Milky Way and Its Satellite, Leo V

  • Signatures of Tidal Disruption in Ultra-Faint Dwarf Galaxies: a Combined HST, Gaia, and MMT/Hectochelle Study of Leo V

    Signatures of Tidal Disruption in Ultra-Faint Dwarf Galaxies: a Combined HST, Gaia, and MMT/Hectochelle Study of Leo V

  • Serendipitous Discovery of RR Lyrae Stars in the Leo V Ultra-Faint Galaxy

    Serendipitous Discovery of RR Lyrae Stars in the Leo V Ultra-Faint Galaxy

  • Marcel S. Pawlowski Phase-Space Structures in Satellite Galaxy Systems

    Marcel S. Pawlowski Phase-Space Structures in Satellite Galaxy Systems

Top View
  • The Observed Properties of Dwarf Galaxies in and Around the Local Group
  • Signals from Dwarf Galaxies
  • Tracer Populations in the Local Group
  • The Enigmatic Pair of Dwarf Galaxies Leo IV and Leo V: Coincidence Or
  • Chemical Abundances of Giant Stars in the Crater Stellar System⋆⋆⋆
  • Pos(DSU 2012)013 (Within the Virial Radius)
  • Leo IV and V – a Possible Dwarf Galaxy Pair?
  • Beasts of the Southern Wild: Discovery of Nine Ultra Faint
  • Pos(INTEGRAL2016)056 ∗ [email protected] Speaker
  • In Pursuit of the Least Luminous Galaxies
  • Signatures of Tidal Disruption in Ultra-Faint Dwarf Galaxies: A
  • The Feeble Giant. Discovery of a Large and Diffuse Milky Way Dwarf Galaxy
  • Ricardo Muñoz the Structural Properties of Milky Way Dwarf
  • Marcel S. Pawlowski Testing Cosmology with Phase-Space
  • Revisiting the Influence of Unidentified Binaries on Velocity Dispersion
  • The Dearth of Neutral Hydrogen in Galactic Dwarf Spheroidal Galaxies
  • Mass First Stars: Importance of Satellite Dwarf Galaxies
  • Arxiv:0807.2831V2 [Astro-Ph] 31 Aug 2008


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