Results 121 to 130 of about 77,155 (253)

Superbubbles in the Magellanic Clouds [PDF]

arXiv, 1998
Superbubbles that result from the stellar winds and supernovae of OB associations probably play a fundamental role in the structure and energetics of the ISM in star-forming galaxies. Their influence may also dominate the relationship between the different interstellar gas phases. How do superbubbles form and evolve?
arxiv  

The Chemical Evolution of the Magellanic Clouds [PDF]

Symposium - International Astronomical Union, 1991
New observations give more details and some confirmation about the chemical evolution of the Clouds. From more numerous data, information is beginning to emerge about the importance of mixing in the Clouds.
F. Spite, M. Spite
openaire   +2 more sources

High Excitation Molecular Gas in the Magellanic Clouds

, 2005
We present the first survey of submillimeter CO 4-3 emission in the Magellanic Clouds. The survey is comprised of 15 6'x6' maps obtained using the AST/RO telescope toward the molecular peaks of the Large and Small Magellanic Clouds.
Alberto D. Bolatto, Chin Y.-N., Christopher L. Martin, Contursi A., Frank P. Israel, Heikkila A., Israel F. P., Israel F. P., Jansen D. J., Johansson L. E. B., Johansson L. E. B., Le Bourlot J., Reach W. T., Rubio M., Rubio M., Rubio M.   +15 more
core   +1 more source

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

The sub-solar Initial Mass Function in the Large Magellanic Cloud

, 2008
The Magellanic Clouds offer a unique variety of star forming regions seen as bright nebulae of ionized gas, related to bright young stellar associations.
Gouliermis, Dimitrios A.
core   +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

Hierarchical star formation in the Magellanic Clouds with the VMC survey. [PDF]

Proc Int Astron Union, 2021
Miller AE, Cioni ML, de Grijs R, Sun NC, VMC Team.   +4 more
europepmc   +1 more source

A Strange Mènage Á Trois [PDF]

arXiv, 2010
The Magellanic Clouds may have joined our Milky Way system quite recently. The Large Magellanic Cloud turns out to be a remarkably luminous object that is close to the upper luminosity limit of the class of magellanic irregular galaxies.
arxiv  

Phosphorus-bearing molecules PO and PN at the edge of the Galaxy. [PDF]

Nature, 2023
Koelemay LA, Gold KR, Ziurys LM.
europepmc   +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