2,824 research outputs found
The X-ray CCD camera of the MAXI Experiment on the ISS/JEM
MAXI, Monitor of All-sky X-ray Image, is the X-ray observatory on the
Japanese experimental module (JEM) Exposed Facility (EF) on the International
Space Station (ISS). MAXI is a slit scanning camera which consists of two kinds
of X-ray detectors: one is a one-dimensional position-sensitive proportional
counter with a total area of , the Gas Slit Camera (GSC), and
the other is an X-ray CCD array with a total area , the
Solid-state Slit Camera (SSC). The GSC subtends a field of view with an angular
dimension of 1 while the SSC subtends a field of view
with an angular dimension of 1 times a little less than 180. In
the course of one station orbit, MAXI can scan almost the entire sky with a
precision of 1 and with an X-ray energy range of 0.5-30 keV. We have
developed the engineering model of CCD chips and the analogue electronics for
the SSC. The energy resolution of EM CCD for Mn K has a full-width at
half maximum of 182 eV. Readout noise is 11 e^- rms.Comment: 10 pages, 4 figures Accepted for Nuclear Instruments and Method in
Physics Researc
Broad Band X-Ray Observations of the Narrow Line X-Ray Galaxy NGC 5506
We present a detailed analysis of broad band X-ray data of the Seyfert 2
galaxy NGC5506. 2-10 keV band are detected during a 1-day ASCA observation,
while no significant change in the 2-10 keV continuum shape is found. The ASCA
spectrum consists of an absorbed power-law, a 'soft excess' below 2 keV, and an
Fe K emission line at 6.4 keV. The 'soft excess' can be well described
by either thermal emission from very low abundance material at a temperature
kT0.8 keV, or scattered/leaking flux from the primary power-law plus a
small amount of thermal emission. Analysis of ROSAT HRI data reveals that the
soft X-ray emission is extended on kpc scales in this object, and the extended
component may account for most of the soft X-ray excess observed by the ASCA.
The result suggests that in this type 2 AGN, the 'soft excess' at least partly
comes from an extended region, imposing serious problem for the model in which
the source is partially covered. Fe K profile is complex and can not be
satisfactorily modeled by a single gaussian. Models of either double gaussians,
or a narrow gaussian plus a line from a relativistic accretion disk viewed at
an inclination of about 40 provide good fits to the data. However,
the inclination of the disk can be substantially larger if there is a small
amount of excessive Fe K edge absorption. The intermediate inclinations for
NLXGs are consistent with the ideas that the inner accretion disk is aligned
with the outer obscuring torus.Comment: 8 pages, 5 postscript figures. to appear in Astrophy. J., 1999, April
2
Electron Density and Temperature Profiles of H-mode Plasma Measured with YAG Thomson Scattering System
Kinetically-balanced Gaussian Basis Set Approach to Relativistic Compton Profiles of Atoms
Atomic Compton profiles (CPs) are a very important property which provide us
information about the momentum distribution of atomic electrons. Therefore, for
CPs of heavy atoms, relativistic effects are expected to be important,
warranting a relativistic treatment of the problem. In this paper, we present
an efficient approach aimed at ab initio calculations of atomic CPs within a
Dirac-Hartree-Fock (DHF) formalism, employing kinetically-balanced Gaussian
basis functions. The approach is used to compute the CPs of noble gases ranging
from He to Rn, and the results have been compared to the experimental and other
theoretical data, wherever possible. The influence of the quality of the basis
set on the calculated CPs has also been systematically investigated.Comment: 31 pages, 12 figure
Magnetic versus nonmagnetic doping effects on the magnetic ordering in the Haldane chain compound PbNi2V2O8
A study of an impurity driven phase-transition into a magnetically ordered
state in the spin-liquid Haldane chain compound PbNi2V2O8 is presented. Both,
macroscopic magnetization as well as 51V nuclear magnetic resonance (NMR)
measurements reveal that the spin nature of dopants has a crucial role in
determining the stability of the induced long-range magnetic order. In the case
of nonmagnetic (Mg2+) doping on Ni2+ spin sites (S=1) a metamagnetic transition
is observed in relatively low magnetic fields. On the other hand, the magnetic
order in magnetically (Co2+) doped compounds survives at much higher magnetic
fields and temperatures, which is attributed to a significant anisotropic
impurity-host magnetic interaction. The NMR measurements confirm the predicted
staggered nature of impurity-liberated spin degrees of freedom, which are
responsible for the magnetic ordering. In addition, differences in the
broadening of the NMR spectra and the increase of nuclear spin-lattice
relaxation in doped samples, indicate a diverse nature of electron spin
correlations in magnetically and nonmagnetically doped samples, which begin
developing at rather high temperatures with respect to the antiferromagnetic
phase transition.Comment: 10 pages, 7 figure
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