2,813 research outputs found
Socialism versus communism: An ethical and psychological contrast
https://stars.library.ucf.edu/prism/1256/thumbnail.jp
Status of the U.S. Academic Research Fleet as Public Vessels under U.S. and International Law
Quasar Jets and their Fields
Observations of jets from quasars and other types of accreting black hole are
briefly summarized. The importance of beaming and -ray observations for
understanding the origin of these jets is emphasised. It is argued that both
the power source and the collimation are likely to be magnetic in origin,
although the details remain controversial. Ultrarelativistic jets may be formed
by the spinning hole and collimated by a hydromagnetic disc wind. Progress in
understanding jets has been handicapped by our inadequate knowledge of how
magnetic field really behaves under cosmic conditions. Fortunately, significant
insights are coming from solar observations, numerical simulation and
laboratory plasma experiments. Some possible, evolutionary ramifications are
briefly discussed and it is suggested that it is the mass of the black hole
relative to that of the galaxy which determines the eventual galaxy morphology.Comment: Latex. 17pages Proc Discusison Meeting on Magnetic Activity in Stars,
Discs and Quasars. Ed. D. Lynden-Bell, E. R. Priest and N. O. Weiss. To
appear in Phil. Trans. Roy. Soc.
Imaging Redshift Estimates for BL Lacertae Objects
We have obtained high dynamic range, good natural seeing i' images of BL
Lacertae objects (BL Lacs) to search for the AGN host and thus constrain the
source redshift. These objects are drawn from a sample of bright flat-spectrum
radio sources that are either known (via recent Fermi LAT observations)
gamma-ray emitters or similar sources that might be detected in continuing
gamma-ray observations. All had spectroscopic confirmation as BL Lac sources,
but no redshift solution. We detected hosts for 25/49 objects. As these
galaxies have been argued to be standard candles, our measured host magnitudes
provide redshift estimates (ranging from 0.2--1.0). Lower bounds are
established on the redshifts of non-detections. The mean of the fit redshifts
(and lower limits) is higher than those of spectroscopic solutions in the
radio- and gamma-ray- loud parent samples, suggesting corrections may be needed
for the luminosity function and evolution of these sources.Comment: 15 pages, to appear in the Astrophysical Journa
Stellar contents and Star formation in the young cluster Stock 18
We have carried out deep (V21 mag) \ubvri photometric study of the star
cluster Stock 18. These along with archival Infrared data have been used to
derive the basic cluster parameters and also to study the star formation
processes in and around the cluster region. The distance to the cluster is
derived as 2.80.2 kpc while its age is estimated as Myr.
Present study indicates that interstellar reddening is normal in the direction
of the cluster. The mass function slope is found to be -1.370.27 for the
mass range 111.9. There is no evidence found for the effect of
mass segregation in main-sequence stars of the cluster. A young stellar
population with age between 1-2 Myr have been found in and around the cluster
region. The presence of IRAS and AKARI sources with MSX intensity map also show
the youth of the Sh2-170 region.Comment: 25 pages, 11 figures, 3 tables (Accepted for publication in New
Astronomy
Yang-Lee and Fisher Zeros of Multisite Interaction Ising Models on the Cayley-type Lattices
A general analytical formula for recurrence relations of multisite
interaction Ising models in an external magnetic field on the Cayley-type
lattices is derived. Using the theory of complex analytical dynamics on the
Riemann sphere, a numerical algorithm to obtain Yang-Lee and Fisher zeros of
the models is developed. It is shown that the sets of Yang-Lee and Fisher zeros
are almost always fractals, that could be associated with Mandelbrot-like sets
on the complex magnetic field and temperature planes respectively.Comment: 9 pages, 3 figures; with minor correction
Perturbation theories for the S=1/2 spin ladder with four-spin ring exchange
The isotropic S=1/2 antiferromagnetic spin ladder with additional four-spin
ring exchange is studied perturbatively in the strong coupling regime with the
help of cluster expansion technique, and by means of bosonization in the weak
coupling limit. It is found that a sufficiently large strength of ring exchange
leads to a second-order phase transition, and the shape of the boundary in the
vicinity of the known exact transition point is obtained. The critical exponent
for the gap is found to be , in agreement both with exact results
available for the dimer line and with the bosonization analysis. The phase
emerging for high values of the ring exchange is argued to be gapped and
spontaneously dimerized. The results for the transition line from strong
coupling and from weak coupling match with each other naturally.Comment: 8 pages, 4 figures, some minor changes in text and reference
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