559 research outputs found
The correlation function of radio sources
We investigate the large-scale clustering of radio sources in the Green Bank
and Parkes-MIT-NRAO 4.85 GHz surveys by measuring the angular two-point
correlation function w(\theta). Excluding contaminated areas, the two surveys
together cover 70 per cent of the whole sky. We find both surveys to be
reasonably complete above 50 mJy. On the basis of previous studies, the radio
sources are galaxies and radio-loud quasars lying at redshifts up to z \sim 4,
with a median redshift z \sim 1. This provides the opportunity to probe
large-scale structures in a volume far larger than that within the reach of
present optical and infrared surveys. We detect a clustering signal w(\theta)
\approx 0.01 for \theta = 1\degr. By assuming an evolving power-law spatial
correlation function in comoving coordinates \xi(r_c,z) = ( r_c / r_0
)^{-\gamma} (1+z)^{\gamma-(3+\epsilon)}, where \gamma = 1.8, and the redshift
distribution N(z) of the radio galaxies, we constrain the r_0--\epsilon
parameter space. For `stable clustering' (\epsilon = 0), we find the
correlation length r_0 \approx 18 Mpc/h, larger than the value for nearby
normal galaxies and comparable to the cluster-cluster correlation length.Comment: 8 pages, 7 ps figures included, LaTeX (mn,sty). Accepted by MNRA
Contributions of point extragalactic sources to the Cosmic Microwave Background bispectrum
All the analyses of Cosmic Microwave Background (CMB) temperature maps
up--to--date show that CMB anisotropies follow a Gaussian distribution. On the
other hand, astrophysical foregrounds which hamper the detection of the CMB
angular power spectrum, are not Gaussian distributed on the sky. Therefore,
they should give a sizeable contribution to the CMB bispectrum. In fact, the
first year data of the Wilkinson Microwave Anisotropy Probe (WMAP) mission have
allowed the {\it first} detection of the extragalactic source contribution to
the CMB bispectrum at 41 GHz and, at the same time, much tighter limits than
before to non--Gaussian primordial fluctuations. In view of the above and for
achieving higher precision in current and future CMB measurements of
non--Gaussianity, in this paper we discuss a comprehensive assessment of the
bispectrum due to either uncorrelated and clustered extragalactic point sources
in the whole frequency interval around the CMB intensity peak. Our
calculations, based on current cosmological evolution models for sources, show
that the reduced angular bispectrum due to point sources, , should be
detectable in all WMAP and Planck frequency channels. We also find agreement
with the results on at 41 GHz coming from the analysis of the first
year WMAP data. Moreover, by comparing with the primordial reduced CMB
bispectrum, we find that only the peak value of the primordial bispectrum
(which appears at ) results greater than in a frequency
window around the intensity peak of the CMB. The amplitude of this window
basically depends on the capability of the source detection algorithms (i.e.,
on the achievable flux detection limit, , for sources).Comment: 26 pages, 6 Figures, use AasTex5.0, ApJ, in press, Oct. 10, 2003
Issu
ASCA observations of the nearby galaxies Dwingeloo 1 and Maffei 1
We present ASCA observations of the nearby galaxies Dwingeloo 1 (Dw1) and
Maffei 1 (Mf1). X-ray sources are clearly detected within 3 arcminutes of the
optical nuclei of both galaxies. Despite the low Galactic latitude of these
fields (|b|<1\degmark) we conclude, on probability and spectral grounds, that
the detected sources are intrinsic to these galaxies rather than foreground or
background interlopers. The Dw1 source, designated Dw1-X1, is interpreted as
being either a hyper-luminous X-ray binary (with a 0.5--10\,keV luminosity of
more than 10^{39}\ergps) or an X-ray bright supernova. The Mf1 emission is
hard and extended, suggesting that it originates from a population of X-ray
binaries. Prompted by the Dw1-X1 results, we discuss the nature of
hyper-luminous X-ray binary systems. Such sources are commonly seen in nearby
galaxies with a frequency of approximately one per galaxy. We present a
possible connection between these luminous systems and Galactic superluminal
sources.Comment: 9 pages (4 ps figures included). Accepted for publication in MNRAS.
Higher quality reproductions of Figure 1 available upon reques
Revisiting glueball wave functions at zero and finite temperature
We study the sizes and thermal properties of glueballs in a three dimensional
compact Abelian gauge model on improved lattice. We predict the radii of and in the units of string tension, or and fm, for the scalar and tensor glueballs, respectively. We perform a well
controlled extrapolation of the radii to the continuum limit and observe that
our results agree with the predicted values. Using Monte Carlo simulations, we
extract the pole-mass of the lowest scalar and tensor glueballs from the
temporal correlators at finite temperature. We see a clear evidence of the
deconfined phase, and the transition appears to be similar to that of the
two-dimensional XY model as expected from universality arguments. Our results
show no significant changes in the glueball wave functions and masses in the
deconfined phase.Comment: 8 pages, 10 figure
Superficial Palmar Arch Aneurysm after Carpal Tunnel Decompression, a Rare Complication: A Case Report
False aneurysms of the palmar arteries are rare. They are usually associated with traumatic injuries to the hand vasculature. We present a case of superficial palmar arch aneurysm (SPAA), complicating carpal tunnel decompression which presented as a pulsatile mass at the site of previous surgery. Initial diagnosis was made on clinical examination and confirmed on doppler ultrasound (US) and computed tomographic angiography (CTA). The feeding vessel of the aneurysm was subsequently occluded using coil embolization
Separable approximation to two-body matrix elements
Two-body matrix elements of arbitrary local interactions are written as the
sum of separable terms in a way that is well suited for the exchange and
pairing channels present in mean-field calculations. The expansion relies on
the transformation to center of mass and relative coordinate (in the spirit of
Talmi's method) and therefore it is only useful (finite number of expansion
terms) for harmonic oscillator single particle states. The converge of the
expansion with the number of terms retained is studied for a Gaussian two body
interaction. The limit of a contact (delta) force is also considered. Ways to
handle the general case are also discussed.Comment: 10 pages, 5 figures (for high resolution versions of some of the
figures contact the author
Synchrotron Emission from Hot Accretion Flows and the Cosmic Microwave Background Anisotropy
Current estimates of number counts of radio sources in the frequency range
where the most sensitive Cosmic Microwave Background (CMB) experiments are
carried out significantly under-represent sources with strongly inverted
spectra. Hot accretion flows around supermassive black holes in the nuclei of
nearby galaxies are expected to produce inverted radio spectra by thermal
synchrotron emission. We calculate the temperature fluctuations and power
spectra of these sources in the Planck Surveyor 30 GHz energy channel, where
their emission is expected to peak. We find that their potential contribution
is generally comparable to the instrumental noise, and approaches the CMB
anisotropy level at small angular scales. Forthcoming CMB missions, which will
provide a large statistical sample of inverted-spectra sources, will be crucial
for determining the distribution of hot accretion flows in nearby quiescent
galactic nuclei. Detection of these sources in different frequency channels
will help constrain their spectral characteristics, hence their physical
properties.Comment: 10 pages, 4 figures, accepted for publication in Ap
Those wonderful elastic waves
We consider in a simple and general way elastic waves in isotropic and
anisotropic media, their polarization, speeds, reflection from interfaces with
mode conversion, and surface waves. Reflection of quasi transverse waves in
anisotropic media from a free surface is shown to be characterized by three
critical angles.Comment: 11 Figures 26 page
An Infrared Determination of the Reddening and Distance to Dwingeloo 1
We present for the first time infrared observations of the nearby highly
obscured galaxy Dwingeloo 1 (Dw1), including deep H-band imaging covering a
total of 4.9x4.9 arcmin, together with J and Ks imaging of the central 2.5x2.5
arcmin. We used the small dispersion of the intrinsic infrared colors of spiral
galaxies to determine an infrared H-band extinction of A_H = 0.47+/-0.11 mag
towards Dw1. In using infrared colors, the uncertainties in the reddening and
distance are reduced by a factor of three. The H-band magnitude corrected for
extinction and the infrared Tully-Fisher relation are then used to estimate a
distance modulus of (m-M)_0 = 28.62+/-0.27, and thus a distance of d = 5.3
{+0.7/-0.6} Mpc, which puts Dw1 at the far end of the IC342/Maffei 1 & 2 group.
Our result is largely independent of the nature of the reddening law because we
estimated both the reddening and the distance at the same wavelength range.Comment: 20 pages, 2 figures, see
http://nicmos2.as.arizona.edu/~aalonso/Dw1/dw1_paper.htm
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