Results 101 to 110 of about 274,720 (148)
Long walk home: Magellanic penguins have strategies that lead them to areas where they can navigate most efficiently. [PDF]
Quintana F+7 more
europepmc +1 more source
NGC1818 unveils the origin of the extended main-sequence turn-off in young Magellanic Clouds clusters. [PDF]
Cordoni G+10 more
europepmc +1 more source
CLSoilMaps: A national soil gridded database of physical and hydraulic soil properties for Chile. [PDF]
Dinamarca DI+3 more
europepmc +1 more source
We present point-source photometry from the Spitzer Space Telescope's final survey of the Small Magellanic Cloud (SMC). We mapped nearly 30 deg ^2 in two epochs in 2017, with the second extending to early 2018 at 3.6 and 4.5 μ m using the Infrared Array ...
T. A. Kuchar+13 more
doaj +1 more source
Sex-specific spatial use of the winter foraging areas by Magellanic penguins and assessment of potential conflicts with fisheries during winter dispersal. [PDF]
Dodino S+5 more
europepmc +1 more source
Extragalactic Science with the Orbiting Astronomical Satellite Investigating Stellar Systems (OASIS) Observatory. [PDF]
Aalto S+7 more
europepmc +1 more source
We investigate the absolute calibration of the tip of the red giant branch (TRGB) in the Small Magellanic Cloud (SMC) using small amplitude red giant stars (SARGs) classified by the Optical Gravitational Lensing Experiment (OGLE).
Nolan W. Koblischke, Richard I. Anderson
doaj +1 more source
We present a catalog of individual stellar and dust extinction properties along close to 500,000 sight lines in the southwest bar of the Small Magellanic Cloud (SMC). The catalog is based on multiband Hubble Space Telescope photometric data spanning near-
Petia Yanchulova Merica-Jones+10 more
doaj +1 more source
The Phanerozoic climate. [PDF]
Shaviv NJ, Svensmark H, Veizer J.
europepmc +1 more source
In the I -band color–magnitude diagrams of resolved nearby galaxies, the reddest asymptotic giant branch ( AGB ) stars form a previously unremarked-upon, but nevertheless distinct and easily identified population of high-luminosity stars.
Barry F. Madore+5 more
doaj +1 more source