8,047 research outputs found
Low-Ionization Emission Regions in Quasars: Gas Properties Probed with Broad O I and Ca II Lines
We have compiled the emission-line fluxes of O I 8446, O I 11287, and the
near-IR Ca II triplet (8579) observed in 11 quasars. These lines are considered
to emerge from the same gas as do the Fe II lines in the low-ionized portion of
the broad emission line region (BELR). The compiled quasars are distributed
over wide ranges of redshift (0.06 < z < 1.08) and of luminosity (-29.8 < M_B <
-22.1), thus representing a useful sample to investigate the line-emitting gas
properties in various quasar environments. The measured line strengths and
velocities, as functions of the quasar properties, are analyzed using
photoionization model calculations. We found that the flux ratio between Ca II
and O I 8446 is hardly dependent on the redshift or luminosity, indicating
similar gas density in the emission region from quasar to quasar. On the other
hand, a scatter of the O I 11287/8446 ratios appears to imply the diversity of
the ionization parameter. These facts invoke a picture of the line-emitting
gases in quasars that have similar densities and are located at regions exposed
to various ionizing radiation fluxes. The observed O I line widths are found to
be remarkably similar over more than 3 orders of magnitude in luminosity, which
indicates a kinematically determined location of the emission region and is in
clear contrast to the well-studied case of H I lines. We also argue about the
dust presence in the emission region since the region is suggested to be
located near the dust sublimation point at the outer edge of the BELR.Comment: Accepted for publication in ApJ; minor rewordings mad
Electron-Electron Interaction in Linear Arrays of Small Tunnel Junctions
We have calculated the spatial distribution of the electrostatic potential
created by an unbalanced charge in one of the conducting electrodes of a
long, uniform, linear array of small tunnel junctions. The distribution
describes, in particular, the shape of a topological single-electron soliton in
such an array. An analytical solution obtained for a circular cross section
model is compared with results of geometrical modeling of a more realistic
structure with square cross section. These solutions are very close to one
another, and can be reasonably approximated by a simple phenomenological
expression. In contrast to the previously accepted exponential approximation,
the new result describes the crossover between the linear change of the
potential near the center of the soliton to the unscreened Coulomb potential
far from the center, with an unexpected ``hump'' near the crossover point.Comment: 8 pages, RevTeX 3.0, 4 PostScript figures. To appear in Applied
Physics Letters, circa 12 Nov 199
A class of Bell diagonal states and entanglement witnesses
We analyze special class of bipartite states - so called Bell diagonal
states. In particular we provide new examples of bound entangled Bell diagonal
states and construct the class of entanglement witnesses diagonal in the magic
basis.Comment: 17 page
Iron-Based Heavy Quasiparticles in SrFeSb: An Infrared Spectroscopic Study
Temperature-dependent infrared reflectivity spectra of SrFeSb
has been measured. A renormalized Drude peak with a heavy effective mass and a
pronounced pseudogap of 10 meV develops in the optical conductivity spectra at
low temperatures. As the temperature decreases below 100 K, the effective mass
() rapidly increases, and the scattering rate () is quenched.
The temperature dependence of and indicates that the
hybridization between the Fe 3d spins and the charge carriers plays an
important role in determining the physical properties of SrFeSb at
low temperatures. This result is the clear evidence of the iron-based heavy
quasiparticles.Comment: 5 pages, 5 figure
OAO/ISLE Near-IR Spectroscopy of IRAS Galaxies
We present the results of the near-infrared (IR) spectroscopy of nine IRAS
galaxies (NGC 1266, NGC 1320, NGC 2633, NGC 2903, NGC 3034, Mrk 33, NGC 7331,
NGC 7625, NGC 7714) with the ISLE imager and spectrograph mounted on the
Okayama Astrophysical Observatory 1.88 m telescope. [Fe II] 1.257 um and Pa
beta emission lines were observed for the whole sample while H2 2.121 um and Br
gamma lines were additionally obtained for two sources, whose flux ratios are
used as a diagnostic tool of dominant energy sources of the galaxies. We find
that the nucleus of NGC 1266 is most likely a low ionization nuclear
emission-line region (LINER), while NGC 2633 and NGC 2903 possibly harbor
active galactic nuclei (AGNs). No AGN or LINER signal is found for other
objects. In addition, we find the spectral features which is indicative of some
unusual phenomena occurring in the galaxies, such as the large [Fe II] line
widths compared to the local escape velocity in NGC 1266. The present work
shows the potential ability of the ISLE to shed new light on the nature of
infrared galaxies, either through a statistical survey of galaxies or an
exploration of spectral features found in individual objects.Comment: Accepted for publication in PAS
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