Magellanic Stream
Top View
- Roman Space Telescope
- THE LOCAL GROUP of GALAXIES* Sidney Van Den Bergh
- Arxiv:1611.04614V1 [Astro-Ph.GA] 14 Nov 2016 Lus Tem N Rde.Rdaigtebupito the of with Blueprint System the Magellanic Redrawing Bridges
- Modelling the Tucana III Stream – a Close Passage with the LMC
- Galaxies AS7007, 2012 Lecture 2: the Milky Way and Local Group
- Follow-Up & Implications of a Recent Star Formation Event Far Into The
- The Four Leading Arms of the Magellanic Cloud System Evidence for Interaction with Milky Way Disk and Halo
- 2020 Symposium – the Local Group
- Remnants of the Sagittarius Dwarf Spheroidal Galaxy Around the Young Globular Cluster Palomar 12
- The Magellanic Stream: Circumnavigating the Galaxy
- THE MAGELLANIC CLOUDS NEWSLETTER an Electronic Publication Dedicated to the Magellanic Clouds, and Astrophysical Phenomena Therein
- They Produced the Nearest Supernova in 300 Years, Are Connected by a Giant Stream of Matter, and May Collide with the Milky Way
- The Magellanic Stream — a Tail of Two Galaxies
- High Velocity Clouds (V > 90 Km/S), up to 108
- Galaxies Through Space and Time Contents INTRODUCTION 4
- David L. Nidever Curriculum Vitae
- The Recent Star-Formation History of the Large and Small Magellanic Clouds
- Arxiv:2012.02649V1 [Astro-Ph.GA] 4 Dec 2020 0.2 Dex and 0.6 Dex, Respectively (Russell & Dopita 1992; the Mcs Are Also Connected by a Mostly Gaseous Rolleston Et Al