Results 241 to 250 of about 222,588 (284)

Orbiting, colliding, and merging liquid lenses on a soap film: Toward gravitational analogs. [PDF]

PNAS Nexus
Martischang JP, Reichert B, Haouche I, Rousseaux G, Duchesne A, Baudoin M.   +5 more
europepmc   +1 more source

Deep phenotyping of an ATDC5 in-vitro cartilage model system. [PDF]

Bone Rep
Klawonn A, Tholen S, Skatulla I, Schröder CM, Arnold SJ, Schilling O, Schmidts M.   +6 more
europepmc   +1 more source

Transport of Electrons in Tangled Magnetic Fields. [PDF]

Space Sci Rev
Verscharen D, Jeffrey N, Artemyev A, Coburn JT, Kunz MW, Pezzi O, Riquelme M, Svenningsson I, Wilson Iii LB.   +8 more
europepmc   +1 more source

SEAL: Spatially-resolved Embedding Analysis with Linked Imaging Data. [PDF]

IEEE Trans Vis Comput Graph
Warchol S, Guo G, Knitte J, Freeman D, Shalla U, Muhlich JL, Sorger PK, Pfister H.   +7 more
europepmc   +1 more source

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The Formation of Galaxies

Physics Today, 1987
Galaxies are beacons that cosmologists use to chart the universe out to its remotest depths. Yet unlike a lighthouse, built on a sturdy pillar of rock, a galaxy resembles an island of light constructed on quicksand in a continuous state of flux. Galaxies are not isolated objects, but are surrounded by close companions, with whom they often maintain ...
openaire   +1 more source

THE FORMATION AND EVOLUTION OF GALAXIES

The New Cosmology, 2005
The past decade has witnessed the establishment of a “standard paradigm” for structure formation in the Universe. It is now universally accepted that the dominant matter component of the Universe is in some form of non-baryonic, weaklyinteracting dark matter. Structure in the dark matter originated from inhomogeneities that were generated shortly after
openaire   +2 more sources

Cosmic strings and the formation of galaxies and clusters of galaxies

Physical Review D, 1986
As many speakers have discussed at this meeting, recent observations of the universe on very large scales have revealed a great deal of structure. Large voids, filaments and sheets with dimensions of 50-100 h-1Mpc stand out in the observed distribution of galaxies. Rich clusters of galaxies are significantly clumped on scales of at least 100 h-1Mpc.
, Turok, , Brandenberger
openaire   +2 more sources

Galaxy Manifolds and Galaxy Formation

1992
We are witnessing the emergence of a physical classification of galaxies. New methods of inquiry, including multivariate statistical analysis of galaxy manifolds, scaling laws and correlations provide important clues towards understanding the formative mechanisms and evolutionary histories of galaxies.
openaire   +2 more sources