Results 131 to 140 of about 30,329 (257)
The proximity of the Magellanic Clouds provides the opportunity to study interacting dwarf galaxies near a massive host, and spatial trends in their stellar population properties in particular, with a unique level of detail.
Roger E. Cohen +13 more
doaj +1 more source
Properties of a Proper-Motion Selected Sample of Giants in the Small Magellanic Cloud Near NGC 121 [PDF]
N. B. Suntzeff +5 more
openalex +1 more source
Obscured Asymptotic Giant Branch stars in the Magellanic Clouds IV. Carbon stars and OH/IR stars [PDF]
J. Th. van Loon +8 more
openalex +1 more source
Cosmic ray feedback in galaxies and galaxy clusters: A pedagogical introduction and a topical review of the acceleration, transport, observables, and dynamical impact of cosmic rays. [PDF]
Ruszkowski M, Pfrommer C.
europepmc +1 more source
We measure the star formation histories (SFHs) from the Scylla survey in ∼98,000 pc ^2 and ∼75,000 pc ^2 of the Small Magellanic Cloud (SMC) and Large Magellanic Cloud (LMC), respectively, using deep Hubble Space Telescope imaging (80% complete to > 1 ...
Clare Burhenne +11 more
doaj +1 more source
The faint Cepheids of the Small Magellanic Cloud: An evolutionary selection effect? [PDF]
Daniel Cordier +2 more
openalex +1 more source
Metallicity Distribution in the LMC and the SMC Based on the Tip-RGB Colors
The color index ( J − K ) _0 of tip-red-giant branch (TRGB) is used to study the metallicity distribution in the Large and Small Magellanic Cloud. With the most complete and pure sample of red member stars so far, the areas are divided into 154 and 70 ...
Ying Li, Biwei Jiang, Yi Ren
doaj +1 more source
SAGE-Spectroscopy: The life-cycle of dust and gas in the Large Magellanic Cloud. Data delivery document v3.0 [PDF]
Paul Woods +5 more
openalex +1 more source

