Results 51 to 60 of about 482,012 (314)

Galactic Density and Evolution Based on the Virial Theorem, Energy Minimization, and Conservation of Angular Momentum

open access: yesGalaxies, 2018
Spiral galaxies are spinning, internally densified objects. The Virial Theorem explains galactic rotation curves via its linkage of the rotation rate to the gravitational self-potential (Ug) and the moment of inertia of oblate spheroids.
Robert E. Criss, Anne M. Hofmeister
doaj   +1 more source

IN-N-OUT: THE GAS CYCLE FROM DWARFS TO SPIRAL GALAXIES [PDF]

open access: yes, 2015
We examine the scalings of galactic outflows with halo mass across a suite of 20 high-resolution cosmological zoom galaxy simulations covering halo masses in the range .
C. Christensen   +7 more
semanticscholar   +1 more source

Mass of Spiral Galaxies by Means of a Maximum Disc Model

open access: yesUniversitas Scientiarum, 2018
Maximum disc mass models for a set of spiral galaxies from the Ursa Major Cluster are presented. We construct the models using the Hunther method and the particular solutions are chosen in such away that the circular velocities are adjusted very ...
Framsol López-Suspes   +1 more
doaj   +1 more source

MAGNETIC FIELDS IN A SAMPLE OF NEARBY SPIRAL GALAXIES [PDF]

open access: yes, 2014
Both observations and modeling of magnetic fields in the diffuse interstellar gas of spiral galaxies are well developed, but the theory has been confronted with observations for only a handful of individual galaxies.
Cameron Van Eck   +3 more
semanticscholar   +1 more source

Gravitational Lensing by Spiral Galaxies [PDF]

open access: yesThe Astrophysical Journal, 1998
27 pages, 7 postscript figures, submitted to ...
Keeton, C. R., Kochanek, C. S.
openaire   +2 more sources

A Catalog of Photometric Redshift and the Distribution of Broad Galaxy Morphologies

open access: yesGalaxies, 2018
We created a catalog of photometric redshift of ∼3,000,000 SDSS galaxies annotated by their broad morphology. The photometric redshift was optimized by testing and comparing several pattern recognition algorithms and variable selection strategies, and ...
Nicholas Paul   +2 more
doaj   +1 more source

Spatial clustering in the ESO-Sculptor Survey: two-point correlation functions by galaxy type at redshifts 0.1 - 0.5 [PDF]

open access: yes, 2007
We calculate the spatial two-point auto and cross-correlation functions for the 765 galaxies with ...
Abazajian   +114 more
core   +4 more sources

THE BLACK HOLE MASS FUNCTION DERIVED FROM LOCAL SPIRAL GALAXIES [PDF]

open access: yes, 2014
We present our determination of the nuclear supermassive black hole (SMBH) mass function for spiral galaxies in the local universe, established from a volume-limited sample consisting of a statistically complete collection of the brightest spiral ...
Benjamin Lee Davis   +8 more
semanticscholar   +1 more source

ULTRALIGHT SCALARS AND SPIRAL GALAXIES [PDF]

open access: yesModern Physics Letters A, 2001
We study some possible astrophysical implications of a very weakly coupled ultralight dilaton-type scalar field. Such a field may develop an (approximately stable) network of domain walls. The domain wall thickness is assumed to be comparable with the thickness of the luminous part of the spiral galaxies. The walls provide trapping for galactic matter.
Dvali, Gia   +2 more
openaire   +2 more sources

Rectangular Spiral Galaxies are still hard

open access: yesComputational Geometry, 2023
Spiral Galaxies is a pencil-and-paper puzzle played on a grid of unit squares: given a set of points called centers, the goal is to partition the grid into polyominoes such that each polyomino contains exactly one center and is 180° rotationally symmetric about its center.
Erik D. Demaine   +2 more
openaire   +5 more sources

Home - About - Disclaimer - Privacy