Results 101 to 110 of about 30,407 (253)

Simulation data for the article "On the Effect of the Large Magellanic Cloud on the Orbital Poles of Milky Way Satellite Galaxies"

open access: green, 2021
Marcel S. Pawlowski   +4 more
openalex   +1 more source

Observations of a Magellanic Corona. [PDF]

open access: yesNature, 2022
Krishnarao D   +8 more
europepmc   +1 more source

III. The Magellanic Clouds [PDF]

open access: yesSymposium - International Astronomical Union, 1959
The Magellanic Clouds offer a unique opportunity to study fully resolved stellar systems at, optical and radio wave-lengths. Optically, with the largest southern telescopes available it is possible to reach absolute magnitudes + 1 to + 2 by direct photography and absolute magnitudes - 6 to - 4 spectroscopically.
openaire   +1 more source

[Nev] Imaging of N49 in the Large Magellanic Cloud [PDF]

open access: green, 2007
Cara E. Rakowski   +2 more
openalex   +1 more source

Stellar Population near NGC 2021: Procession of Star Formation in the South Rim of Supergiant Shell LMC 4

open access: yesThe Astronomical Journal
Supergiant shells (SGSs) are the largest interstellar structures where heated and enriched gas flows into the host galaxy’s halo. The SGSs in the Large Magellanic Cloud (LMC) are so close that their stars can be resolved with ground-based telescopes to ...
Po-Sheng Ou   +4 more
doaj   +1 more source

Obscured Asymptotic Giant Branch stars in the Magellanic Clouds III. New IRAS counterparts [PDF]

open access: green, 1997
J. Th. van Loon   +5 more
openalex   +1 more source

Star formation in the Magellanic clouds [PDF]

open access: yes
Because of their proximity, the Magellanic Clouds provide the opportunity to conduct a detailed study of the history and current state of star formation in dwarf irregular galaxies. There is considerable evidence that star formation in the Clouds was and
Frogel, Jay A.
core   +1 more source

Magellanic Cloud Planetary Nebulae [PDF]

open access: yesProceedings of the International Astronomical Union, 2006
Over the past 15 years the growth of detailed information about Planetary Nebulae in the Large and Small Magellanic Clouds (MCPN) has been explosive, to the point where these galactic laboratories are the preferred context for furthering and refining our understanding of this late phase of stellar evolution.
openaire   +1 more source

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