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Leo I (dwarf galaxy)

  • Distribution of Phantom Dark Matter in Dwarf Spheroidals Alistair O

    Distribution of Phantom Dark Matter in Dwarf Spheroidals Alistair O

  • Searching for Diffuse Light in the M96 Group

    Searching for Diffuse Light in the M96 Group

  • Is There Tension Between Observed Small Scale Structure and Cold Dark Matter?

    Is There Tension Between Observed Small Scale Structure and Cold Dark Matter?

  • The Hubble Space Telescope Proper Motion Collaboration HSTPROMO

    The Hubble Space Telescope Proper Motion Collaboration HSTPROMO

  • Calendar of Roman Events

    Calendar of Roman Events

  • The Beginners Guide to Astrology AQUARIUS JAN

    The Beginners Guide to Astrology AQUARIUS JAN

  • Hubble Space Telescope Observations of the Local Group

    Hubble Space Telescope Observations of the Local Group

  • Streaming Motion in Leo I

    Streaming Motion in Leo I

  • Neutral Hydrogen in Local Group Dwarf Galaxies

    Neutral Hydrogen in Local Group Dwarf Galaxies

  • Searches for HI in the Outer Parts of Four Dwarf Spheroidal Galaxies

    Searches for HI in the Outer Parts of Four Dwarf Spheroidal Galaxies

  • Galaxy Group and Cluster Astronomy at RIT

    Galaxy Group and Cluster Astronomy at RIT

  • Dissecting the Stellar Content of Leo I: a Dwarf Irregular Caught in Transition

    Dissecting the Stellar Content of Leo I: a Dwarf Irregular Caught in Transition

  • 7. Dwarf Galaxies

    7. Dwarf Galaxies

  • Environmental Influences on Dwarf Galaxy Evolution: the Group Environment

    Environmental Influences on Dwarf Galaxy Evolution: the Group Environment

  • Arxiv:1411.4053V1 [Astro-Ph.GA] 14 Nov 2014 That Mass Loss Plays an Important Part in Stellar Evolu- 5 IAASARS, National Observatory of Athens, GR-15236 Pen- Tion

    Arxiv:1411.4053V1 [Astro-Ph.GA] 14 Nov 2014 That Mass Loss Plays an Important Part in Stellar Evolu- 5 IAASARS, National Observatory of Athens, GR-15236 Pen- Tion

  • The Darkest Galaxies

    The Darkest Galaxies

  • Did Leo I Collide with the Magellanic Clouds?

    Did Leo I Collide with the Magellanic Clouds?

  • Lesson 13: Comparison of Numbers Written in Scientific Notation and Interpreting Scientific Notation Using Technology

    Lesson 13: Comparison of Numbers Written in Scientific Notation and Interpreting Scientific Notation Using Technology

Top View
  • Leo a Monthly Guide to the Night Sky by Tom Trusock
  • Exploring the Decans
  • Signals from Dwarf Galaxies
  • The Local High-Redshift Dwarf Galaxies
  • Globular Cluster Systems and Galaxy Halo Masses
  • The Dynamics and Metallicity Distribution of the Distant Dwarf Galaxy Vv124∗
  • HST Observations of the Local Group Dwarf Galaxy Leo I
  • Astro-Ph/9807296
  • 98 New Study Denies Dark Matter's Role in Dwarf Galaxies
  • Elemental Abundance Distributions of Milky Way Satellite Galaxies
  • Ricardo Muñoz the Structural Properties of Milky Way Dwarf
  • Powerpoint Slides
  • Luis A. Ureña-López Department of Physics, University of Guanajuato
  • The MEDIDO Project: Surprising Result for Leo I
  • BST1047+ 1156: an Extremely Diffuse and Gas-Rich Object in the Leo I Group
  • Arxiv:0906.2178V1 [Astro-Ph.CO] 11 Jun 2009 Prtdudrcoeaieareetb Soitduniver Associated by Agreement Inc
  • Vettius Valens, Anthologies, Book I
  • The Dearth of Neutral Hydrogen in Galactic Dwarf Spheroidal Galaxies


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