Results 1 to 10 of about 30,329 (257)
NGC1818 unveils the origin of the extended main-sequence turn-off in young Magellanic Clouds clusters [PDF]
The nature of young star clusters in the Magellanic Clouds is debated. Here, the authors show an alternative approach that exploits data to exclude the presence of age differences greater than a few million years among cluster stars in a very young ...
Giacomo Cordoni +10 more
doaj +2 more sources
Magellanic Clouds: I. Transparency. [PDF]
Shapley H.
europepmc +4 more sources
Magellanic Clouds: VI. Revised Distances and Luminosities. [PDF]
Shapley H.
europepmc +4 more sources
Magellanic Clouds: V. Fifty Eclipsing Stars. [PDF]
Shapley H, Nail VM.
europepmc +4 more sources
Magellanic Clouds: IV. On the Period Frequency Anomalies. [PDF]
Shapley H, Nail VM.
europepmc +4 more sources
Discovery of the Magellanic Stellar Stream Out to 100 kpc
The Magellanic Stream (MS)—an enormous ribbon of gas spanning 140° of the southern sky trailing the Magellanic Clouds—has been exquisitely mapped in the five decades since its discovery.
Vedant Chandra +9 more
doaj +1 more source
Magellanic Clouds Cepheids: Thorium Abundances [PDF]
The analysis of the high-resolution spectra of 31 Magellanic Clouds Cepheid variables enabled the identification of thorium lines. The abundances of thorium were found with spectrum synthesis method. The calculated thorium abundances exhibit correlations
Yeuncheol Jeong +5 more
doaj +1 more source
Magellanic Clouds: VIII. On the Population Characteristics of the Two Clouds. [PDF]
Shapley H.
europepmc +4 more sources
The Magellanic Stream and the Magellanic Cloud System [PDF]
A tidal model has been introduced to the triple system of the Galaxy, Large and Small Magellanic Clouds (the LMC and SMC hereafter) and successfully reproduced the Magellanic Stream (Murai and Fujimoto 1980; Lin and Lynden-Bell 1982; Gardiner et al. 1994; Gardiner and Noguchi 1995; Lin et al. 1995), a narrow band of diffuse atomic hydrogen gas emerging
M. Fujimoto, T. Sawa, Y. Kumai
openaire +1 more source
The relation between radio flux density and ionizing ultra-violet flux for HII regions and supernova remnants in the Large Magellanic cloud [PDF]
We present a comparison between the Parkes radio surveys (Filipović et al 1995) and Vacuum Ultra-Violet (VUV) surveys (Smith et al. 1987) of the Large Magellanic Clouds (LMC). We have found 72 sources in common in the LMC which are known HII regions (52)
Filipović M.D., Jones P.A., Vhite G.L.
doaj +1 more source

