Results 61 to 70 of about 29,924 (195)
Cold neutral hydrogen (H i ) is a crucial precursor for molecular gas formation and can be studied via H i absorption. This study investigates H i absorption in low column density regions of the Small and Large Magellanic Clouds (SMC and LMC) using the ...
Hongxing Chen +20 more
doaj +1 more source
Hierarchical star formation in the Magellanic Clouds with the VMC survey. [PDF]
Miller AE +4 more
europepmc +1 more source
We present the first systematic analysis comparing the ages, reddening, and radial velocities of star clusters using two widely used tools: STARLIGHT and Analyzer of Spectra for Age Determination (A.S.A.D). Both tools utilize the full integrated spectrum
Martina I. Tapia-Reina +3 more
doaj +1 more source
Effects of Metallicity on the Rotation Rates of Massive Stars
Recent theoretical predictions for low metallicity massive stars predict that these stars should have drastically reduced equatorial winds (mass loss) while on the main sequence, and as such should retain most of their angular momentum.
Amanda J. Sprague +7 more
core +2 more sources
Phosphorus-bearing molecules PO and PN at the edge of the Galaxy. [PDF]
Koelemay LA, Gold KR, Ziurys LM.
europepmc +1 more source
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 +15 more
doaj +1 more source
The VISCACHA survey – II. Structure of star clusters in the Magellanic Clouds periphery [PDF]
J. F. C. Santos +13 more
openalex +1 more source
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 +4 more
doaj +1 more source
Observations of a Magellanic Corona. [PDF]
Krishnarao D +8 more
europepmc +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

