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Pisces II (dwarf galaxy)
Wyn Evans Institute of Astronomy, Cambridge
Spatial Distribution of Galactic Globular Clusters: Distance Uncertainties and Dynamical Effects
Galactic Archaeology. the Dwarfs That Survived and Perished
What Is an Ultra-Faint Galaxy?
Searching for Dark Matter Annihilation in Recently Discovered Milky Way Satellites with Fermi-Lat A
Draft181 182Chapter 10
N.W. Evans (Cambridge)
The Pristine Dwarf-Galaxy Survey – II
Galaxies on Sub-Galactic Scales
Watkins Laura.Pdf (PDF, 5Mb)
Atlases and Catalogues a Revised Shapley Ames Catalog, 195, 258
Gaia DR2 Proper Motions of Dwarf Galaxies Within 420 Kpc Orbits, Milky Way Mass, Tidal Influences, Planar Alignments, and Group Infall
– 1 – Table 1. Basic Information
Marcel S. Pawlowski Phase-Space Structures in Satellite Galaxy Systems
The Observed Properties of Dwarf Galaxies in and Around the Local Group
1506.01021V1.Pdf
Tracer Populations in the Local Group
Galactic Forces Rule the Dynamics of Milky Way Dwarf Galaxies
Top View
Physics/Astronomy
Galaxy Formation & Evolution
Arxiv:2105.11488V1 [Astro-Ph.GA] 24 May 2021 We Observe Today Is Still a Very Hot Topic of Modern Astronomy
Vasily Belokurov, Institute of Astronomy, Cambridge UK Pairing Dark Matter Halos and Astrophysical Objects
Horologium Ii: a Second Ultra-Faint Milky Way Satellite in the Horologium Constellation
Ricardo Muñoz the Structural Properties of Milky Way Dwarf
The New Milky Way Satellites: Alignment with the VPOS and Predictions for Proper Motions and Velocity Dispersions
A CEMP-No Star in the Ultra-Faint Dwarf Galaxy Pisces II? M
FY15 High-Level Deliverables
How Massive Are the Least Massive Galaxies?
The Milky Way's Neighbours Observed with GLAO
Marcel S. Pawlowski Testing Cosmology with Phase-Space
The Dearth of Neutral Hydrogen in Galactic Dwarf Spheroidal Galaxies
Gaia Early DR3 Systemic Motions of Local Group Dwarf Galaxies and Orbital Properties with a Massive Large Magellanic Cloud
Mass First Stars: Importance of Satellite Dwarf Galaxies
Arxiv:1802.06810V1 [Astro-Ph.GA] 19 Feb 2018 Identify 4 Member Stars, from Which We Calculate a Systemic Velocity of Vhel = 284.6−3.1 Km S
Mapping Stellar Substructure in the Milky Way Bound & Unbound
A CEMP-No Star in the Ultra-Faint Dwarf Galaxy Pisces II
Speller Ryan.Pdf (2.871Mb)
A Timeline of the Decans: from Egyptian Astronomical
Big Fish, Small Fish: Two New Ultra-Faint Satellites of the Milky