Results 121 to 130 of about 22,251 (204)

Mass-loss Rate of Highly Evolved Stars in the Magellanic Clouds

open access: yesThe Astrophysical Journal Supplement Series
Asymptotic giant branch stars (AGBs) and red supergiant stars (RSGs) exhibit significant mass-loss phenomena and are considered important sources of interstellar dust.
Jing Wen   +5 more
doaj   +1 more source

Unraveling the Kinematic and Morphological Evolution of the Small Magellanic Cloud

open access: yesThe Astrophysical Journal
We model the kinematics of the Small Magellanic Cloud (SMC) by analyzing the proper motions (PMs) from Gaia DR3 of nine different stellar populations, including young main-sequence (MS) stars (
S. R. Dhanush   +2 more
doaj   +1 more source

NGC1818 unveils the origin of the extended main-sequence turn-off in young Magellanic Clouds clusters. [PDF]

open access: yesNat Commun, 2022
Cordoni G   +10 more
europepmc   +1 more source

Long walk home: Magellanic penguins have strategies that lead them to areas where they can navigate most efficiently. [PDF]

open access: yesProc Biol Sci, 2022
Quintana F   +7 more
europepmc   +1 more source

ALMA Observations of Molecular Complexity in the Large Magellanic Cloud: Probing the Star-forming Region N 160

open access: yesThe Astrophysical Journal
Hot cores are small (≲0.1 pc), dense (≥10 ^6 cm ^−3 ), and hot (>100 K) regions around massive protostars and are one of the main production sites of complex organic molecules (COMs, ≥6 atoms, including carbon).
Amanda Broadmeadow   +11 more
doaj   +1 more source

Modeling of Granulation in Red Supergiants in the Magellanic Clouds with the Gaussian Process Regressions

open access: yesThe Astrophysical Journal
The granulation of red supergiants (RSGs) in the Magellanic Clouds is systematically investigated by combining the latest RSG samples and light curves from the Optical Gravitational Lensing Experiment and the All-Sky Automated Survey for Supernovae.
Zehao Zhang   +4 more
doaj   +1 more source

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