2,731 research outputs found
ASCA Observation of the Lyman-limit Quasar PKS2145+067
X-ray observation of a famous Lyman-limit quasar PKS2145+067at z_em= 0.990
was carried with ASCA. The source showed a 2-10 keV flux of 1.3 E-11 erg cm^-2
sec^-1 (L_X = 2.5 E46 erg sec^-1 for H_0=50 km s^-1 Mpc^-1) described by a
power-law spectrum with a photon index Gamma=1.63 +/- 0.04 . In the ASCA energy
band, no excess absorption was detected implying the absorption column density
at z_ ab=0.791 was less than 1.6 E21 cm^-2 if absorbing medium had a metal
abundance of 0.5 solar. Comparison with previous Einstein and ROSAT
observations shows that PKS2145+067 has increased its luminosity by a factor of
2--3 between 1991 and 1998.Comment: 15 pages, 3figures, Latex(PASJadd,sty, PASJ95.sty) accepted in PAS
XMM-Newton Observation of IC 310 in the Outer Region of the Perseus Cluster of Galaxies
We present results from an XMM-Newton observation of the head-tail radio
galaxy IC 310 located in the southwest region of the Perseus cluster. The
spectrum is well-fitted by an absorbed power-law model with a photon index of
with no significant absorption excess. The X-ray image shows a
point-like emission at IC 310 without any signs of a structure correlated with
the radio halo tail. The temperature of the intracluster medium surrounding IC
310 declines as a function of distance from the cluster center, from keV in the northeast corner of the field of view to about 3 keV in the
southwest region. Although we do not find any sharp edges in the surface
brightness profile, a brightness excess over a smooth model by about
20% is seen. The temperature also rises by about 10% in the same region. This
indicates that the IC 310 region is a subcluster probably infalling into the
Perseus cluster, and the gas in front of IC 310 towards the Perseus cluster is
likely to be compressed by the large-scale motion, which supports the view that
the IC 310 system is undergoing a merger.Comment: 7 pages, 8 figures (including color), accepted for publication in
PAS
Chandra observation of the core of the galaxy cluster AWM7
We present results from a Chandra observation of the core region of the
nearby X-ray bright galaxy cluster AWM7. There are blob-like substructures,
which are seen in the energy band 2--10 keV, within 10 kpc (20'') of the cD
galaxy NGC1129, and the brightest sub-peak has a spatial extent more than 4
kpc. We also notice that the central soft X-ray peak is slightly offset from
the optical center by 1 kpc. These structures have no correlated features in
optical, infrared, or radio band. Energy spectrum of the hard sub-peak
indicates a temperature higher than 3 keV with a metallicity less than 0.3
solar, or a power-law spectrum with photon index 1.2. A hardness ratio map and
a narrow Fe-K band image jointly indicate two Fe-rich blobs symmetrically
located around the cD galaxy, with the direction perpendicular to the sub-peak
direction. In larger scales (r<60 kpc), the temperature gradually drops from 4
keV to 2 keV toward the cluster center and the metal abundance rises steeply to
a peak of 1.5 solar at r=7 kpc. These results indicate that a dynamical process
is going on in the central region of AWM7, which probably creates heated gas
blobs and drives metal injection.Comment: 12 pages, 7 figures (including color), accepted for publication in
ApJ. Postscript is also available at
http://www-x.phys.metro-u.ac.jp/~furusho/papers.htm
DIOS: the dark baryon exploring mission
DIOS (Diffuse Intergalactic Oxygen Surveyor) is a small satellite aiming for
a launch around 2020 with JAXA's Epsilon rocket. Its main aim is a search for
warm-hot intergalactic medium with high-resolution X-ray spectroscopy of
redshifted emission lines from OVII and OVIII ions. The superior energy
resolution of TES microcalorimeters combined with a very wide field of view
(30--50 arcmin diameter) will enable us to look into gas dynamics of cosmic
plasmas in a wide range of spatial scales from Earth's magnetosphere to
unvirialized regions of clusters of galaxies. Mechanical and thermal design of
the spacecraft and development of the TES calorimeter system are described. We
also consider revising the payload design to optimize the scientific capability
allowed by the boundary conditions of the small mission.Comment: 10 pages, 11 figures, Proceedings of the SPIE Astronomical
Instrumentation : Space Telescopes and Instrumentation 2014: Ultraviolet to
Gamma Ra
Electrically driven spin excitation in a ferroelectric magnet DyMnO_3
Temperature (5--250 K) and magnetic field (0--70 kOe) variations of the
low-energy (1--10 meV) electrodynamics of spin excitations have been
investigated for a complete set of light-polarization configurations for a
ferroelectric magnet DyMnO by using terahertz time-domain spectroscopy. We
identify the pronounced absorption continuum (1--8 meV) with a peak feature
around 2 meV, which is electric-dipole active only for the light -vector
along the a-axis. This absorption band grows in intensity with lowering
temperature from the spin-collinear paraelectric phase above the ferroelectric
transition, but is independent of the orientation of spiral spin plane ( or
), as shown on the original (ferroelectric polarization)
phase as well as the magnetic field induced phase. The possible origin of this electric-dipole active band is argued in
terms of the large fluctuations of spins and spin-current.Comment: New version, 11 pages including colored 8 figure
Locating the Warm-Hot Intergalactic Medium in the Simulated Local Universe
We present an analysis of mock spectral observation of warm-hot intergalactic
medium (WHIM) using a constrained simulation of the local universe. The
simulated map of oxygen emission lines from local WHIM reproduces well the
observed structures traced by galaxies in the real local universe. We further
attempt to perform mock observations of outer parts of simulated Coma cluster
and A3627 adopting the expected performance of DIOS (Diffuse Intergalactic
Oxygen Surveyor), which is proposed as a dedicated soft X-ray mission to search
for cosmic missing baryons. We find that WHIMs surrounding nearby clusters are
detectable with a typical exposure time of a day, and thus constitute realistic
and promising targets for DIOS. We also find that an X-ray emitting clump in
front of Coma cluster, recently reported in the XMM-Newton observation, has a
counterpart in the simulated local universe, and its observed spectrum can be
well reproduced in the simulated local universe if the gas temperature is set
to the observationally estimated value.Comment: 25 pages, 3 tables, 16 figures. Accepted for publication in PASJ.
High resolution PS/PDF files are available at
http://www-utap.phys.s.u-tokyo.ac.jp/~kohji/research/x-ray/index.htm
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