Results 101 to 110 of about 30,329 (257)

Scylla. III. The Outside-in Radial Age Gradient in the Small Magellanic Cloud and the Star Formation Histories of the Main Body, Wing, and Outer Regions

The Astrophysical Journal
The proximity of the Large and Small Magellanic Clouds (LMC and SMC) provides the opportunity to study the impact of dwarf–dwarf interactions on their mass assembly with a unique level of detail. To this end, we analyze two-filter broadband imaging of 83
Roger E. Cohen, Kristen B. W. McQuinn, Claire E. Murray, Benjamin F. Williams, Yumi Choi, Christina W. Lindberg, Clare Burhenne, Karl D. Gordon, Petia Yanchulova Merica-Jones, Caroline Bot, Andrew E. Dolphin, Karoline M. Gilbert, Steven Goldman, Alec S. Hirschauer, Karin M. Sandstrom, O. Grace Telford   +15 more
doaj   +1 more source

Multiwavelength Period–Luminosity and Period–Luminosity–Color Relations at Maximum Light for Mira Variables in the Magellanic Clouds [PDF]

, 2019
Anupam Bhardwaj, Shashi M. Kanbur, Shiyuan He, M. Rejkuba, Noriyuki Matsunaga, Richard de Grijs, Kaushal Kumar Sharma, Harinder P. Singh, Tapas Baug, Chow‐Choong Ngeow, J. Ou   +10 more
openalex   +1 more source

Observations of a Magellanic Corona. [PDF]

Nature, 2022
Krishnarao D, Fox AJ, D'Onghia E, Wakker BP, Cashman FH, Howk JC, Lucchini S, French DM, Lehner N.   +8 more
europepmc   +1 more source

III. The Magellanic Clouds [PDF]

Symposium - 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

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

The 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, Rui-Ching Chao, You-Hua Chu, Chin-Yi Hsu, Chuan-Jui Li   +4 more
doaj   +1 more source

EROS2 microlensing search towards the Magellanic Clouds [PDF]

, 1999
T. Lasserre, Collaboration, EROS
openalex   +1 more source

Magellanic Cloud Planetary Nebulae [PDF]

Proceedings 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

Dust around red supergiants in the Magellanic Clouds [PDF]

, 2008
Geoffrey C. Clayton, William R. Freeman, Stacey N. Bright, Philip Massey, Karl D. Gordon, Emily M. Levesque, B. Plez, Knut Olsen, Jason Nordhaus   +8 more
openalex   +1 more source

Star formation in the Magellanic clouds [PDF]

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

Identifying H i Emission and UV Absorber Associations near the Magellanic Stream

The Astrophysical Journal
We present a new technique to identify associations of H i emission in the Magellanic Stream (MS) and ultraviolet (UV) absorbers from 92 QSO sight lines near the MS. We quantify the level of associations of individual H i elements to the main H i body of
Doyeon A. Kim, Yong Zheng, Mary E. Putman   +2 more
doaj   +1 more source