Results 81 to 90 of about 274,720 (148)

Untangling Magellanic Streams

open access: yesThe Open Journal of Astrophysics
The Magellanic Stream (MS) is known to contain multiple HI strands and corresponding stellar populations are being discovered. Combining a sample of 17 stars from the H3 (“Hectochelle in the Halo at High Resolution”) survey with 891 stars drawn from the
Dennis Zaritsky   +5 more
doaj   +1 more source

Scylla. II. The Spatially Resolved Star Formation History of the Large Magellanic Cloud Reveals an Inverted Radial Age Gradient

open access: yesThe Astrophysical Journal
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

Carbonaceous dust grains seen in the first billion years of cosmic time. [PDF]

open access: yesNature, 2023
Witstok J   +41 more
europepmc   +1 more source

Infrared Dark Clouds in the Small Magellanic Cloud?

open access: yes, 2009
We have applied the unsharp-masking technique to the 24 $\mu$m image of the Small Magellanic Cloud (SMC), obtained with the Spitzer Space Telescope, to search for high-extinction regions.
Alberto D. Bolatto   +57 more
core   +1 more source

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

Observations of a Magellanic Corona. [PDF]

open access: yesNature, 2022
Krishnarao D   +8 more
europepmc   +1 more source

Effects of Metallicity on the Rotation Rates of Massive Stars

open access: yes, 2004
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

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

A Radio and Optical Polarization Study of the Magnetic Field in the Small Magellanic Cloud

open access: yes, 2008
We present a study of the magnetic field of the Small Magellanic Cloud (SMC), carried out using radio Faraday rotation and optical starlight polarization data.
B. M. Gaensler   +25 more
core   +1 more source

The Distant Milky Way Halo from the Southern Hemisphere: Characterization of the LMC-induced Dynamical Friction Wake

open access: yesThe Astrophysical Journal
The infall of the Large Magellanic Cloud (LMC) into the Milky Way’s halo impacts the distribution of stars and dark matter (DM) in our Galaxy. Mapping the observational consequences of this encounter can inform us about the properties of both galaxies ...
Manuel Cavieres   +8 more
doaj   +1 more source

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