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Magellanic Stream
HI in the M31/M33 Environment
ASKAP and Meerkat Surveys of the Magellanic Clouds
Revealing the Ionization Properties of the Magellanic Stream Using Optical Emission
NASA Program & Budget Update
On the Magellanic Stream, the Mass of the Galaxy and the Age of the Universe
The Dynamics of the Galaxies in the Local Group Roeland Van Der Marel (Stsci)
E+FW Abstract Book
THE MAGELLANIC CLOUDS NEWSLETTER an Electronic Publication Dedicated to the Magellanic Clouds, and Astrophysical Phenomena Therein
The Dynamics of the Galaxies in the Local Group
III. Star Clusters Counterpart of the Magellanic Bridge and Counter-Bridge in 8D?
Young Stars Raining Through the Galactic Halo: the Nature and Orbit of Price-Whelan 1 Michele Bellazzini, Rodrigo Ibata, Nicolas F
Arxiv:Astro-Ph/0307509V1 29 Jul 2003 Rpittpstuigl Using Typeset Preprint Hl 02 N Speitdb Iuain Fte“Cosmic the of Simulations by Davé Predicted (E.G
The Magellanic Stream As a Probe of Astrophysics
The Magellanic Corona and the Formation of the Magellanic Stream
The Magellanic Stream: the 'Ram Pressure Plus Collision'
THE MAGELLANIC STREAM and the DENSITY of CORONAL GAS in the GALACTIC HALO ABSTRACT the Properties of the Magellanic Stream Const
OUR SOLAR SYSTEM Realms of Fire and Ice We Start Your Tour of the Cosmos with Gas and Ice Giants, a Lot of Rocks, and the Only Known Abode for Life
THE MAGELLANIC CLOUDS NEWSLETTER an Electronic Publication Dedicated to the Magellanic Clouds, and Astrophysical Phenomena Therein
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
The Magellanic Stream*
The Kinematics of the Tucana Dwarf Galaxy
THE ORIGIN of the MAGELLANIC STREAM and ITS LEADING ARM David L
Arxiv:Astro-Ph/9401008V1 7 Jan 1994
Beyond Our Galaxy: the Local Group
H I Kinematics of the Large Magellanic Cloud Revisited
The Many Streams of the Magellanic Stream
New Quasars Behind the Magellanic Clouds. Spectroscopic Confirmation
The Large Magellanic Cloud Stellar Content with SMASH I
Fossil Imprint of a Powerful Flare at the Galactic Centre Along the Magellanic Stream
The Magellanic Stream
MILKY WAY Turns out to Be a Dynamic, Living Object
Roman Space Telescope
Arxiv:2108.08310V1 [Astro-Ph.GA] 18 Aug 2021 of Gas (Both Neutral and Ionized, Fox Et Al