Results 61 to 70 of about 470,379 (288)

On the maximum value of the cosmic abundance of oxygen and the oxygen yield [PDF]

open access: yes, 2007
We search for the maximum oxygen abundance in spiral galaxies. Because this maximum value is expected to occur in the centers of the most luminous galaxies, we have constructed the luminosity - central metallicity diagram for spiral galaxies, based on a ...
Allende Prieto   +68 more
core   +1 more source

SPIN ALIGNMENTS OF SPIRAL GALAXIES WITHIN THE LARGE-SCALE STRUCTURE FROM SDSS DR7 [PDF]

open access: yes, 2014
Using a sample of spiral galaxies selected from the Sloan Digital Sky Survey Data Release 7 and Galaxy Zoo 2, we investigate the alignment of spin axes of spiral galaxies with their surrounding large-scale structure, which is characterized by the large ...
Youcai Zhang   +8 more
semanticscholar   +1 more source

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

Nuclear Spirals in Galaxies [PDF]

open access: yes, 2008
6 pages, 4 figures, to appear in ""Mapping the Galaxy and Nearby Galaxies", Eds. K. Wada and F.
openaire   +3 more sources

The optical polarization of spiral galaxies [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2000
Scattering of starlight by dust, molecules and electrons in spiral galaxies will produce a modification of the direct intensity and a polarization in the observed light. We treat the case where the distribution of scatterers can be considered to be optically thin, and derive semi-analytic expressions for the resolved intensity and polarized intensity ...
Edouard Audit, John F. L. Simmons
openaire   +4 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

Assembling Spiral Galaxies [PDF]

open access: yesSymposium - International Astronomical Union, 1996
Nearby spiral galaxies offer vital clues to some of the most fundamental questions about galaxy formation and evolution: What is the star formation history of the universe, past and future? When did disks form, during the final stages of a single primeval collapse, or as a continuous or episodic process?
openaire   +2 more sources

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.
Gregory Gabadadze   +2 more
openaire   +4 more sources

Extragalactic Magnetism with SOFIA (SALSA Legacy Program). V. First Results on the Magnetic Field Orientation of Galaxies

open access: yesThe Astrophysical Journal, 2023
We present the analysis of the magnetic field ( B -field) structure of galaxies measured with far-infrared (FIR) and radio (3 and 6 cm) polarimetric observations.
Alejandro S. Borlaff   +15 more
doaj   +1 more source

Gravitational Instability of Gas–Dust Circumnuclear Disks in Galaxies

open access: yesGalaxies, 2023
We numerically study the origin of the multi-armed spiral structure observed in the circumnuclear gaseous mini-disks of nearby galaxies. We show that the presence of dust in such disks and its interaction with the gravitationally stable gaseous component
Roman Tkachenko   +2 more
doaj   +1 more source

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