Results 81 to 90 of about 144,718 (240)
Magnetic-Field Vector Maps of Nearby Spiral Galaxies
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
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]
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]
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
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
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
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
23 pages, LaTeX, SISSA Ref.
GIURICIN G+3 more
openaire +4 more sources
Stellar Populations in Spiral Galaxies [PDF]
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]
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