187 research outputs found
A new approach to the reduction of "Carte du Ciel" plates
A new procedure for the reduction of "Carte du Ciel" plates is presented. A
typical "Carte du Ciel" plate corresponding to the Bordeaux zone has been taken
as an example. It shows triple exposures for each object and the modelling of
the data has been performed by means of a non-linear least squares fitting of
the sum of three bivariate Gaussian distributions. A number of solutions for
the problems present in this kind of plates (optical aberrations, adjacency
photographic effects, presence of grid lines, emulsion saturation) have been
investigated. An internal accuracy of 0.1'' in x and y was obtained for the
position of each of the individual exposures. The external reduction to a
catalogue led to results with an accuracy of 0.16'' in x and 0.13'' in y for
the mean position of the three exposures. A photometric calibration has also
been performed and magnitudes were determined with an accuracy of 0.09 mags.Comment: 10 pages, 12 enclosed post-script figures, uses l-aa.sty (included).
Accepted for publication in Astronomy and Astrophysics Supp. Serie
Scaling Relations for Collision-less Dark Matter Turbulence
Many scaling relations are observed for self-gravitating systems in the
universe. We explore the consistent understanding of them from a simple
principle based on the proposal that the collision-less dark matter fluid terns
into a turbulent state, i.e. dark turbulence, after crossing the caustic
surface in the non-linear stage. The dark turbulence will not eddy dominant
reflecting the collision-less property. After deriving Kolmogorov scaling laws
from Navier-Stokes equation by the method similar to the one for Smoluchowski
coagulation equation, we apply this to several observations such as the
scale-dependent velocity dispersion, mass-luminosity ratio, magnetic fields,
and mass-angular momentum relation, power spectrum of density fluctuations.
They all point the concordant value for the constant energy flow per mass: , which may be understood as the speed of the hierarchical
coalescence process in the cosmic structure formation.Comment: 26 pages, 6 figure
Binding Energy and the Fundamental Plane of Globular Clusters
A physical description of the fundamental plane of Galactic globular clusters
is developed which explains all empirical trends and correlations in a large
number of cluster observables and provides a small but complete set of truly
independent constraints on theories of cluster formation and evolution in the
Milky Way. Within the theoretical framework of single-mass, isotropic King
models, it is shown that (1) 39 regular (non--core-collapsed) globulars with
measured core velocity dispersions share a common V-band mass-to-light ratio of
1.45 +/- 0.10, and (2) a complete sample of 109 regular globulars reveals a
very strong correlation between cluster binding energy and total luminosity,
regulated by Galactocentric position: E_b \propto (L^{2.05} r_{\rm gc}^{-0.4}).
The observational scatter about either of these two constraints can be
attributed fully to random measurement errors, making them the defining
equations of a fundamental plane for globular clusters. A third, weaker
correlation, between total luminosity and the King-model concentration
parameter, c, is then related to the (non-random) distribution of globulars on
the plane. The equations of the FP are used to derive expressions for any
cluster observable in terms of only L, r_{\rm gc}, and c. Results are obtained
for generic King models and applied specifically to the globular cluster system
of the Milky Way.Comment: 60 pages with 19 figures, submitted to Ap
Some Aspects of Rotational and Magnetic Energies for a Hierarchy of Celestial Objects
Celestial objects, from earth like planets to clusters of galaxies, possess
angular momentum and magnetic fields. Here we compare the rotational and
magnetic energies of a whole range of these celestial objects together with
their gravitational self energies and find a number of interesting
relationships. The celestial objects, due to their magnetic fields, also posses
magnetic moments. The ratio of magnetic moments of these objects with the
nuclear magnetic moments also exhibits interesting trends. We also compare
their gyromagnetic ratio which appears to fall in a very narrow range for the
entire hierarchy of objects. Here we try to understand the physical aspects
implied by these observations and the origin of these properties in such a wide
range of celestial objects, spanning some twenty orders in mass, magnetic field
and other parameters.Comment: 12 pages, 37 equation
A GLIMPSE into the Nature of Galactic Mid-IR Excesses
We investigate the nature of the mid-IR excess for 31 intermediate-mass stars
that exhibit an 8 micron excess in either the Galactic Legacy Infrared
Mid-Plane Survey Extraordinaire or the Mid-Course Space Experiment using high
resolution optical spectra to identify stars surrounded by warm circumstellar
dust. From these data we determine projected stellar rotational velocities and
estimate stellar effective temperatures for the sample. We estimate stellar
ages from these temperatures, parallactic distances, and evolutionary models.
Using MIPS [24] measurements and stellar parameters we determine the nature of
the infrared excess for 19 GLIMPSE stars. We find that 15 stars exhibit Halpha
emission and four exhibit Halpha absorption. Assuming that the mid-IR excesses
arise in circumstellar disks, we use the Halpha fluxes to model and estimate
the relative contributions of dust and free-free emission. Six stars exhibit
Halpha fluxes that imply free-free emission can plausibly explain the infrared
excess at [24]. These stars are candidate classical Be stars. Nine stars
exhibit Halpha emission, but their Halpha fluxes are insufficient to explain
the infrared excesses at [24], suggesting the presence of a circumstellar dust
component. After the removal of the free-free component in these sources, we
determine probable disk dust temperatures of Tdisk~300-800 K and fractional
infrared luminosities of L(IR)/L(*)~10^-3. These nine stars may be
pre-main-sequence stars with transitional disks undergoing disk clearing. Three
of the four sources showing Halpha absorption exhibit circumstellar disk
temperatures ~300-400 K, L(IR)/L(*)~10^-3, IR colors K-[24]< 3.3, and are warm
debris disk candidates. One of the four Halpha absorption sources has K-[24]>
3.3 implying an optically thick outer disk and is a transition disk candidate.Comment: 17 figures. Accepted for publication in Ap
The Worst Distortions of Astrometric Instruments and Orthonormal Models for Rectangular Fields of View
The non-orthogonality of algebraic polynomials of field coordinates
traditionally used to model field-dependent corrections to astrometric
measurements, gives rise to subtle adverse effects. In particular, certain
field dependent perturbations in the observational data propagate into the
adjusted coefficients with considerable magnification. We explain how the worst
perturbation, resulting in the largest solution error, can be computed for a
given non-orthogonal distortion model. An algebraic distortion model of full
rank can be converted into a fully orthonormal model based on the Zernike
polynomials for a circular field of view, or a basis of functions constructed
from the original model by a variant of the Gram-Schmidt orthogonalization
process for a rectangular field of view. The relative significance of
orthonormal distortion terms is assessed simply by the numerical values of the
corresponding coefficients. Orthonormal distortion models are easily extendable
when the distribution of residuals indicate the presence of higher order terms.Comment: 1 figure; submitted in PAS
Astrometry and geodesy with radio interferometry: experiments, models, results
Summarizes current status of radio interferometry at radio frequencies
between Earth-based receivers, for astrometric and geodetic applications.
Emphasizes theoretical models of VLBI observables that are required to extract
results at the present accuracy levels of 1 cm and 1 nanoradian. Highlights the
achievements of VLBI during the past two decades in reference frames, Earth
orientation, atmospheric effects on microwave propagation, and relativity.Comment: 83 pages, 19 Postscript figures. To be published in Rev. Mod. Phys.,
Vol. 70, Oct. 199
Cosmology, Oscillating Physics and Oscilllating Biology
According to recent reports there is an excess correlation and an apparent
regularity in the galaxy one-dimensional polar distribution with a
characteristic scale of 128 Mpc. This aparent spatial periodicity can
be naturally explained by a time oscillation of the gravitational constant .
On the other hand, periodic growth features of bivalve and coral fossiles
appear to show a periodic component in the time dependence of the number of
days per year. In this letter we show that a time oscillating gravitational
constant with similar period and amplitude can explain such a feature.Comment: 9 pages. latex using revtex. This revised version is supposed to be
free of e-mail nois
Relict periglacial soils on Quaternary terraces in the central Ebro Basin (NE Spain)
Pedofeatures associated with ancient cold climatic conditions have been recognized in soils on terraces in the Monegros area (central Ebro Basin, Spain), at a latitude of 41°49âČN and an altitude of 300 m a.s.l. Eleven soil profiles were described on fluvial deposits corresponding to the most extensive terrace (T5) of the Alcanadre River, Middle Pleistocene in age (MIS8âMIS7). Each soil horizon was sampled for physical, chemical, mineralogical and micromorphological analyses. Macromorphological features related to pedocryogenic processes were described: involutions, jacked stones, shattered stones, detached and vertically oriented carbonatic pendents, fragmented carbonatic crusts, laminar microstructures, succitic fabric, silt cappings on rock fragments and aggregates, and irregular, broken, discontinuous and deformed gravel and sandy pockets. Accumulations of FeâMn oxides, dissolution features on the surface of carbonatic stones, and calcitic accumulations were identified related to vadoseâphreatic conditions. The observed periglacial features developed under cold environmental conditions in exceptional geomorphic and hydrological conditions. This soil information may have potential implications in studies of paleoclimate in the Ebro Valley as well as in other Mediterranean areas
Rotation Curve of Galaxies by the Force Induced by Mass of Moving Particles
We suggest that there is a novel force which is generated by the mass of
relatively moving particles. The new force which we named Mirinae Force is a
counterpart of the magnetic force operating between electrically charged moving
particles. Instead of using the conventional dark matter, we applied the
mirinae force to a particular model system of the spiral galaxy in which most
of the galaxy's mass is located within the central region where some portion of
the inner mass is in revolving motion at a relativistic speed. The calculation
yielded three important results that illustrate the existence of mirinae force
and validate the proposed model: First, the mirinae force in this model
explains why most of the matters in the galactic disk are in the circular
motion which is similar to cycloid. Second, the mirinae force well explains not
only the flat rotation curve but also the varied slope of the rotation curve
observed in the spiral galaxies. Third, at the flat velocity of 220 Km/s, the
inner mass of the Milky Way calculated by using the proposed model is
6.0\times10^11 M\odot, which is very close to 5.5\times10^11 M\odot (r <50 Kpc,
including Leo I) estimated by using the latest kinematic information. This
means that the mirinae force well takes the place of the dark matter of the
Milky Way
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