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Bound star clusters observed in a lensed galaxy 460 Myr after the Big Bang. [PDF]
Adamo A +27 more
europepmc +1 more source
ABSTRACT Over the years, numerous D‐ and z‐values have been published in the scientific literature. While these values initially appear to be valid criteria for assessing and comparing the heat resistance of different microorganisms under the same conditions or the same microorganism under different conditions, this is not always the case.
Astrid Gędas, Agnes Weiss
wiley +1 more source
The effect of nanohydroxyapatite serum and toothpaste on prevention of enamel demineralization around orthodontic brackets: an in vitro study. [PDF]
Babanouri N +3 more
europepmc +1 more source
Bridging Flocculation of a Sterically Stabilized Cationic Latex as a Biosensor for the Detection of Microbial DNA after Amplification via PCR. [PDF]
Trinh E +5 more
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Monitoring of Bicelles Spreading into Floating Lipid Bilayers. [PDF]
Bożek J +4 more
europepmc +1 more source
Galaxy Tomography with the Gravitational Wave Background from Supermassive Black Hole Binaries
Chen Y.
europepmc +1 more source
A dynamically young and perturbed Milky Way disk [PDF]
The evolution of the Milky Way disk, which contains most of the stars in the Galaxy, is affected by several phenomena. For example, the bar and the spiral arms of the Milky Way induce radial migration of stars and can trap or scatter stars close to orbital resonances.
Dafydd Wyn Evans, Eloisa Poggio
exaly +10 more sources
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The Milky Way disk non‐axisymmetries and galactoseismology
Astronomische Nachrichten, 2016AbstractCurrent Galactic dynamical models still most often rely on the assumptions of a smooth time‐independent and axisymmetric gravitational potential. On the other hand, ab initio simulations in a cosmological context are not very flexible to precisely produce a model of our own Galaxy, or to disentangle the internal and the external/environmental ...
Famaey, Benoit +2 more
openaire +1 more source
EVOLUTION OF THE MILKY WAY DISK
2006The Solar neighbourhood is where the physical basis for models of the evolu- tion of spiral galaxy disks can be tested most stringently. A new survey has provided full space motions, metallicities, ages, and duplicity information for over 14,000 nearby F and G dwarfs.
Nordström, Birgitta, Andersen, Johannes
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