Results 111 to 120 of about 30,812 (255)

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

Cepheid mass-luminosity relations from the Magellanic Clouds [PDF]

, 2001
J. P. Beaulieu, J. R. Buchler, Z. Kolláth   +2 more
openalex   +1 more source

New probable planetary nebulae and VV Cephei stars in the Small Magellanic Cloud [PDF]

, 1981
N. Sanduleak, Peter Pesch
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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

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

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

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

The mass-loss rates of red supergiants at low metallicity: detection of rotational CO emission from two red supergiants in the Large Magellanic Cloud [PDF]

, 2016
M. Matsuura, B. A. Sargent, B. M. Swinyard, J. Yates, P. Royer, M. J. Barlow, Martha L. Boyer, L. Decin, T. Khouri, M. Meixner, J. Th. van Loon, Paul Woods   +11 more
openalex   +1 more source

Ages and metallicities of five intermediate-age star clusters projected towards the Small Magellanic Cloud [PDF]

, 2001
Andrés E. Piatti, J. F. C. Santos, Joan Clària, E. Bica, Ata Sarajedini, D. Geisler   +5 more
openalex   +1 more source

Nearby primitive galaxies offer a window into the early universe. [PDF]

Proc Natl Acad Sci U S A, 2022
Croswell K.
europepmc   +1 more source