5 research outputs found
Origin of Galactic and Extragalactic Magnetic Fields
A variety of observations suggest that magnetic fields are present in all
galaxies and galaxy clusters. These fields are characterized by a modest
strength (10^{-7}-10^{-5} G) and huge spatial scale (~Mpc). It is generally
assumed that magnetic fields in spiral galaxies arise from the combined action
of differential rotation and helical turbulence, a process known as the
alpha-omega dynamo. However fundamental questions concerning the nature of the
dynamo as well as the origin of the seed fields necessary to prime it remain
unclear. Moreover, the standard alpha-omega dynamo does not explain the
existence of magnetic fields in elliptical galaxies and clusters. The author
summarizes what is known observationally about magnetic fields in galaxies,
clusters, superclusters, and beyond. He then reviews the standard dynamo
paradigm, the challenges that have been leveled against it, and several
alternative scenarios. He concludes with a discussion of astrophysical and
early Universe candidates for seed fields.Comment: 67 pages, 17 figures, accepted for publication in Reviews of Modern
Physic
A
We present observations of the 12CO(J=1-0) line at 2.6 mm
of 65 galaxies located in the Coma supercluster region: 33
actually belong to the Coma supercluster while 32 are either
foreground or background objects. These data have been obtained
using the NRAO 12 m telescope at Kitt Peak (United States), and
for four galaxies, using the IRAM 30 m telescope at Pico Veleta
(Spain). Out of these 65 galaxies, 54 had never been observed in
the CO(1-0) line; 49 have been detected by us, of which 37 are
new detections. We give molecular gas masses deduced from the CO
line integrated intensities, and upper limits for the 16
undetected objects, computed with a Galactic conversion factor
N() = 2.3 1020
I(CO) and H0 = 75 km/s/Mpc
<SUP>12</SUP>CO(1-0) observation of isolated late-type galaxies
International audienceWe present 12CO(J=1-0) line observations of 99 galaxies obtained with the SEST 15 m, the Kitt Peak 12 m and the IRAM 30 m telescopes. The target galaxies were selected from the catalogue of isolated galaxies of Karachentseva (\cite{Karachentseva73}). These data are thus representative of the CO properties of isolated late-type galaxies. All objects were observed in their central position, those with large angular sizes were mapped. These new measurements are used to estimate the molecular gas mass of the target galaxies. The molecular gas is on average ~ 18% of the atomic gas mass. Tables 1 and 2 are also available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/411/381 Based on observations made with the 12-m National Radio Astronomical Observatory, Kitt Peak, Arizona, with the Swedish-ESO Submillimetre telescope SEST, La Silla, Chile, with the IRAM 30 m radiotelescope, Pico Veleta, Granada, Spain