Results 81 to 90 of about 144,718 (240)

Magnetic-Field Vector Maps of Nearby Spiral Galaxies

open access: yesGalaxies, 2019
We present a method for determining the directions of magnetic-field vectors in a spiral galaxy using two synchrotron polarization maps, an optical image, and a velocity field.
Hiroyuki Nakanishi   +2 more
doaj   +1 more source

Atmospheric Pressure and Molecular Cloud Formation in Early-type Galaxies

open access: yesThe Astrophysical Journal, 2023
A strong correlation between atmospheric pressure and molecular gas mass is found in central cluster galaxies and early-type galaxies. This trend and a similar trend with atmospheric gas density would naturally arise if the molecular clouds condensed ...
Iu. V. Babyk   +5 more
doaj   +1 more source

Multiple Mechanisms Quench Passive Spiral Galaxies [PDF]

open access: yes, 2017
We examine the properties of a sample of 35 nearby passive spiral galaxies in order to determine their dominant quenching mechanism(s). All five low mass ($\textrm{M}_{\star} < 1 \times 10^{10} \textrm{M}_{\odot}$) passive spiral galaxies are located in the rich Virgo cluster.
arxiv   +1 more source

A multi-wavelength study of spiral structure in galaxies. I. General characteristics in the optical [PDF]

open access: yes, 2020
Different spiral generation mechanisms are expected to produce different morphological and kinematic features. In this first paper in a series we carefully study the parameters of spiral structure in 155 face-on spiral galaxies, selected from the Sloan Digital Sky Survey, in the three $gri$ bands.
arxiv   +1 more source

Rotating shallow water modeling of planetary,astrophysical and plasma vortical structures (plasma transport across a magnetic field,model of the jupiter's GRS, prediction of existence of giant vortices in spiral galaxies)

open access: yesDiscrete Dynamics in Nature and Society, 1999
Three kinds of results have been described in this paper. Firstly, an experimental study of the Rossby vortex meridional drift on the rotating shallow water has been carried out.
M. V. Nezlin   +4 more
doaj   +1 more source

Subarcminute Localization of 13 Repeating Fast Radio Bursts Detected by CHIME/FRB

open access: yesThe Astrophysical Journal, 2023
We report on improved sky localizations of 13 repeating fast radio bursts (FRBs) discovered by CHIME/FRB via the use of interferometric techniques on channelized voltages from the telescope.
Daniele Michilli   +29 more
doaj   +1 more source

Multi‐Modal Instrument Performances (MMIP): A Musical Database

open access: yesComputer Graphics Forum, EarlyView.
Abstract Musical instrument performances are multimodal creative art forms that integrate audiovisual elements, resulting from musicians' interactions with instruments through body movements, finger actions, and facial expressions. Digitizing such performances for archiving, streaming, analysis, or synthesis requires capturing every element that shapes
T. Kyriakou   +2 more
wiley   +1 more source

The local galaxy density and the bars of spiral galaxies

open access: yesThe Astrophysical Journal, 1993
23 pages, LaTeX, SISSA Ref.
GIURICIN G   +3 more
openaire   +4 more sources

Stellar Populations in Spiral Galaxies [PDF]

open access: yesProceedings of the International Astronomical Union, 2006
We report preliminary results of the characterization of bulge and inner disk stellar populations for 8 nearby spiral galaxies using Gemini/GMOS. The long-slit spectra extend out to 1-2 disk scale lengths with S/N/Ang > 50. Two different model fitting techniques, absorption-line indices and full spectral synthesis, are found to weigh age ...
J. Jesús González   +2 more
openaire   +3 more sources

Color Differences between Clockwise and Counterclockwise Spiral Galaxies [PDF]

open access: yesarXiv, 2013
While spiral galaxies observed from Earth clearly seem to spin in different directions, little is yet known about other differences between galaxies that spin clockwise and galaxies that spin counterclockwise. Here we compared the color of 64,399 spiral galaxies that spin clockwise to 63,215 spiral galaxies that spin counterclockwise.
arxiv  

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