7,118 research outputs found
Variable stars in the globular cluster NGC 3201. I. Multimode SX Phe-type variables
We report on the discovery of eleven multimode SX Phoenicis--type blue
stragglers in the field of the southern globular cluster NGC 3201. In these
variables both radial and non-radial modes are excited. For three variables the
derived period ratio is close to that observed in SX Phoenicis itself,
suggesting that these stars are pulsating in the fundamental and the
first-overtone radial modes. Using the McNamara (1997) period-luminosity
relation we have estimated the apparent distance modulus to NGC 3201 to be
14.08mag.Comment: 10 pages, requires mn2e.cls,contact the first author at
[email protected] for high-resolution figure
Twisting commutative algebraic groups
If is a commutative algebraic group over a field , is a
commutative ring that acts on , and is a finitely generated free
-module with a right action of the absolute Galois group of , then there
is a commutative algebraic group over , which is a twist of
a power of . These group varieties have applications to cryptography (in the
cases of abelian varieties and algebraic tori over finite fields) and to the
arithmetic of abelian varieties over number fields. For purposes of such
applications we devote this article to making explicit this tensor product
construction and its basic properties.Comment: To appear in Journal of Algebra. Minor changes from original versio
Anharmonic Torsional Stiffness of DNA Revealed under Small External Torques
DNA supercoiling plays an important role in a variety of cellular processes.
The torsional stress related with supercoiling may be also involved in gene
regulation through the local structure and dynamics of the double helix. To
check this possibility steady torsional stress was applied to DNA in the course
of all-atom molecular dynamics simulations. It is found that small static
untwisting significantly reduces the torsional persistence length () of
GC-alternating DNA. For the AT-alternating sequence a smaller effect of the
opposite sign is observed. As a result, the measured values are similar
under zero stress, but diverge with untwisting. The effect is traced to
sequence-specific asymmetry of local torsional fluctuations, and it should be
small in long random DNA due to compensation. In contrast, the stiffness of
special short sequences can vary significantly, which gives a simple
possibility of gene regulation via probabilities of strong fluctuations. These
results have important implications for the role of local DNA twisting in
complexes with transcription factors.Comment: 8 pages, 5 figures, to appear in Phys. Rev. Let
NGC 4654: polarized radio continuum emission as a diagnostic tool for a galaxy--cluster interaction
A recent comparison between deep VLA HI observations and dynamical models of
the Virgo cluster spiral galaxy NGC 4654 has shown that only a model involving
a combination of a tidal interaction and ram pressure can reproduce the data.
Deep radio polarization studies, together with detailed MHD modeling, can
independently verify those conclusions, that are based on HI observations and
dynamical models. We performed deep polarized radio-continuum observations of
the Virgo cluster spiral galaxy NGC 4654 with the Effelsberg 100m telescope at
8.35 GHz and the VLA at 4.85 GHz. Detailed 3D MHD simulations were made to
determine the large-scale magnetic field and the emission distribution of the
polarized radio continuum in the model, during the galaxy evolution within the
cluster environment. This direct comparison between the observed and simulated
polarized radio continuum emission corroborates the earlier results, that the
galaxy had a recent rapid close encounter with NGC 4639 and is undergoing weak
ram pressure by the intracluster medium. This combination of deep radio
polarization studies and detailed MHD modeling thus gives us unique insight
into the interactions of a galaxy with its cluster environment. It represents a
diagnostic tool that is complementary to deep HI observations.Comment: Corrected galaxy name in captions of figures (1 & 2
Are There Topological Black Hole Solitons in String Theory?
We point out that the celebrated Hawking effect of quantum instability of
black holes seems to be related to a nonperturbative effect in string theory.
Studying quantum dynamics of strings in the gravitational background of black
holes we find classical instability due to emission of massless string
excitations. The topology of a black hole seems to play a fundamental role in
developing the string theory classical instability due to the effect of sigma
model instantons. We argue that string theory allows for a qualitative
description of black holes with very small masses and it predicts topological
solitons with quantized spectrum of masses. These solitons would not decay into
string massless excitations but could be pair created and may annihilate also.
Semiclassical mass quantization of topological solitons in string theory is
based on the argument showing existence of nontrivial zeros of beta function of
the renormalization group.Comment: 12 pages, TeX, requires phyzzx.tex, published in Gen. Rel. Grav. 19
(1987) 1173; comment added on December 18, 199
Comparison of FDMA and CDMA for second generation land-mobile satellite communications
Code Division Multiple Access (CDMA) and Frequency Division Multiple Access (FDMA) (both analog and digital) systems capacities are compared on the basis of identical link availabilities and physical propagation models. Parameters are optimized for a bandwidth limited, multibeam environment. For CDMA, the benefits of voice activated carriers, antenna discrimination, polarization reuse, return link power control and multipath suppression are included in the analysis. For FDMA, the advantages of bandwidth efficient modulation/coding combinations, voice activated carriers, polarization reuse, beam placement, and frequency staggering were taken into account
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