Results 181 to 190 of about 612,026 (282)
Were All Massive Stars Born in OB Associations and Clusters? [PDF]
It has been commonly conjectured that all massive >10 Msun stars are born in OB associations or clusters. Many O and B stars in the Galaxy or the Magellanic Clouds appear to exist in isolation, however. While some of these field OB stars have been ejected from their birthplaces, some are too far away from massive star forming regions to be runaways ...
arxiv
The surface distribution clusters, planetary nebulae, supergiant M stars, and carbon stars in the Large Magellanic Cloud [PDF]
B. E. Westerlund
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A cluster of intermediate age in the Large Magellanic Cloud [PDF]
Richard Woolley
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A Census of Dwarf Galaxy Satellites around LMC-mass Galaxy NGC 2403
We present the first comprehensive census of the satellite population around a Large Magellanic Cloud stellar-mass galaxy, as part of the Magellanic Analog Dwarf Companions and Stellar Halos (MADCASH) survey. We have surveyed NGC 2403 ( D = 3.0 Mpc) with
Jeffrey L. Carlin+13 more
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Nearby primitive galaxies offer a window into the early universe. [PDF]
Croswell K.
europepmc +1 more source
A New and Unusual Variable Star in the Large Magellanic Cloud [PDF]
Frances W. Wright, P. W. Hodge
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The Metallicities of Five Small High-velocity Clouds
High-velocity clouds (HVCs) are multiphase gas structures whose velocities (∣ v _LSR ∣ ≥ 100 km s ^−1 ) are too high to be explained by Galactic disk rotation.
Trisha Ashley+7 more
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Long walk home: Magellanic penguins have strategies that lead them to areas where they can navigate most efficiently. [PDF]
Quintana F+7 more
europepmc +1 more source
THE MAGELLANIC CLOUDS. XIV. THE BAR OF THE LARGE CLOUD [PDF]
Virginia McKibben Nail, Harlow Shapley
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The infall of the Large Magellanic Cloud (LMC) into the Milky Way’s halo impacts the distribution of stars and dark matter (DM) in our Galaxy. Mapping the observational consequences of this encounter can inform us about the properties of both galaxies ...
Manuel Cavieres+8 more
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