Results 1 to 10 of about 849,819 (226)

Magellanic Stream: A Possible Tool for Studying Dark Halo Model [PDF]

, 2005
Hosein Haghi, Akram Hasani Zonoozi, S. Rahvar   +2 more
openalex   +1 more source

On the formation of the Magellanic Stream [PDF]

, 2003
C. Mastropietro, Ben Moore, Lucio Mayer, Joachim Stadel, James Wadsley   +4 more
openalex   +1 more source

Spectral types in the direction of the Magellanic Stream [PDF]

, 1982
E. Recillas-Cruz
openalex   +1 more source

On the Distance of the Magellanic Stream [PDF]

, 1984
J. Jaaniste
openalex   +1 more source

A Pre-Infall Magellanic Analog-Corona and Stream formation in the \textsc{HESTIA} cosmological simulations [PDF]

R. M. Chisholm, Elena D’Onghia, Noam I. Libeskind, Scott Lucchini, Andrew J. Fox, Matthias Steinmetz   +5 more
openalex   +1 more source

An estimate of the mass of the Milky Way from the Magellanic Stream

Monthly notices of the Royal Astronomical Society, 2021
We present a model for the formation of the Magellanic Stream (MS) due to ram pressure stripping. We model the history of the Small and Large Magellanic Clouds in the recent cosmological past in a static Milky Way potential with diffuse halo gas, using
P. Craig, S. Chakrabarti, S. Baum, Benjamin T Lewis   +3 more
semanticscholar   +1 more source

Exploring the Mysteries of the Magellanic Stream: What We’ve Uncovered and What Remains Unknown

Proceedings of the International Astronomical Union, 2023
The Magellanic Stream is a lengthy, ribbon-like gas structure stretching 200 degrees across the sky and surrounding the Large and Small Magellanic Clouds. These two galaxies are the brightest dwarf galaxies orbiting the Milky Way (MW).
Elena D’Onghia
semanticscholar   +1 more source

Stingrays in the radio sky: Two unusual diffuse radio relic sources in the direction of the Magellanic Stream

Publications Astronomical Society of Australia
We present the discovery of two extended, low surface-brightness radio continuum sources, each consisting of a near-circular body and an extended tail of emission, nicknamed Stingray 1 (ASKAP J0129–5350) and Stingray 2 (ASKAP J0245–5642).
Z. Smeaton, M. Filipović, B. Koribalski, M. Sasaki, R. Alsaberi, A. Bradley, E. J. Crawford, Shi Dai, Nikhel Gupta, F. Haberl, Andrew M. Hopkins, T. Jarrett, S. Lazarevi'c, D. Leahy, P. Macgregor, Gavin Rowell, S. Shabala, D. Urošević, J. V. van Loon, T. Vernstrom   +19 more
semanticscholar   +1 more source

The Magellanic Stream

Publications of the Astronomical Society of Australia, 1976
I shall briefly outline some observational aspects of the Magellanic Stream before discussing the pros and cons of the two conflicting theories of its origin: a) that the Stream was pulled out of the Clouds by tidal forces produced by a close encounter with our Galaxy and b) that the gas clouds of the Stream are primordial and in the same orbit as the ...
openaire   +1 more source

Following the tidal trail: a history of modeling the Magellanic Stream

Astrophysics and Space Science
The formation of the Magellanic Stream has puzzled astronomers for decades. In this review, we outline the history of our understanding of the Magellanic System highlighting key observations that have revolutionized thinking of its evolution.
Scott Lucchini
semanticscholar   +1 more source