Canis Major Overdensity
Top View
- Annual Report 2008
- Instituto De Astrofísica De Andalucía - Consejo Superior De Investigaciones Científicas Investigador Principal Emilio J
- Evolution Over Time of the Milky Way's Disc Shape
- Dwarf Galaxy Planes: the Discovery of Symmetric Structures in the Local Group
- Stellar Streams and Clouds in the Galactic Halo 3 2 Currently Known Stellar Debris Streams and Clouds in the Galactic Halo
- Why the Canis Major Overdensity Is Not Due to the Warp: Analysis of Its Radial Profile and Velocities N
- The AAT/WFI Survey of the Monoceros Ring and Canis Major Dwarf Galaxy 3 Gion Should Provide Strong Indications If a Dwarf Galaxy Resides in the Plane Or Not
- The Asiago Red Clump Spectroscopic Survey and Its First Applications
- Galaxies 626
- The Aquarius Comoving Group Is Not a Disrupted Classical Globular Cluster
- SCYON Issue 58
- Milky Way Halo Objects IC 4499 and the Large Magellanic Cloud
- Quantitative Maps of Stellar Substructures in the Milky Way Jelte De Jong Quantitative Maps of Stellar Substructures in the Milky Way
- UVES Observations of the Canis Major Overdensity The
- Spectral Results for the Blue Plume Stars in Canis Major Overdensity
- 01 Front Matter ASSEMBLY.Pages
- Space Exploration & Space Colonization Handbook
- The Canis Major Dwarf Galaxy