996 research outputs found
Promoted Sulfated Zirconia: Modification of Zirconia Bulk through Incorporation of Fe and Mn Cations
High Resolution Infrared Imaging of the Compact Nuclear Source in NGC4258
We present high resolution imaging of the nucleus of NGC4258 from 1 micron to
18 microns. Our observations reveal that the previously discovered compact
source of emission is unresolved even at the near-infrared resolution of about
0.2 arcsec FWHM which corresponds to about 7 pc at the distance of the galaxy.
This is consistent with the source of emission being the region in the
neighborhood of the purported 3.5*10^7 M_sun black hole. After correcting for
about 18 mags of visual extinction, the infrared data are consistent with a
F_nu \propto nu^(-1.4+/-0.1) spectrum from 1.1 micron to 18 micron, implying a
non-thermal origin. Based on this spectrum, the total extinction corrected
infrared luminosity (1-20 micron) of the central source is 2*10^8 L_sun. We
argue that the infrared spectrum and luminosity of the central source obviates
the need for a substantial contribution from a standard, thin accretion disk at
these wavelengths and calculate the accretion rate through an advection
dominated accretion flow to be Mdot \sim 10^(-3) M_sun/yr. The agreement
between these observations and the theoretical spectral energy distribution for
advection dominated flows provides evidence for the existence of an advection
dominated flow in this low luminosity AGN.Comment: 21 pages, 5 figures, Appearing in Mar 2000 ApJ vol. 53
HRTEM observation of the monoclinic-to-tetragonal (m-t) phase transition in nanocrystalline ZrO<sub>2</sub>
The orientation relations m(100) || t(001), m[001] || t[110]; m(011) || t(100), m[001] || t[110]; m(100) || t(110), m[001] || t[001]; m(013) || t(116), m[001] || t[001]; (indices for the primitive tetragonal cell) have been found between the tetragonal (t) and monoclinic (m) domains during the electron irradiation-induced m-t phase transition observed in-situ with HREM within isolated zirconia nanoparticles. Geometric models of the m-t interfaces are proposed. Keywords High-resolution transmission electron microscopy, nanoparticles, orientation relations, polymorphism, zirconia, catalys
The Mid-Infrared Instrument for the James Webb Space Telescope, VIII: The MIRI Focal Plane System
We describe the layout and unique features of the focal plane system for
MIRI. We begin with the detector array and its readout integrated circuit
(combining the amplifier unit cells and the multiplexer), the electronics, and
the steps by which the data collection is controlled and the output signals are
digitized and delivered to the JWST spacecraft electronics system. We then
discuss the operation of this MIRI data system, including detector readout
patterns, operation of subarrays, and data formats. Finally, we summarize the
performance of the system, including remaining anomalies that need to be
corrected in the data pipeline
High Spatial Resolution Imaging of NGC 1068 in the Mid Infrared
Mid-infrared observations of the central source of NGC 1068 have been
obtained with a spatial resolution in the deconvolved image of 0.1" (~ 7pc).
The central source is extended by ~1" in the north-south direction but appears
unresolved in the east-west direction over most of its length. About two-thirds
of its flux can be ascribed to a core structure which is itself elongated
north-south and does not show a distinct unresolved compact source. The source
is strongly asymmetric, extending significantly further to the north than to
the south. The morphology of the mid-infrared emission appears similar to that
of the radio jet, and has features which correlate with the images in [O III].
Its 12.5-24.5 micron color temperature ranges from 215 to 260 K and does not
decrease smoothly with distance from the core. Silicate absorption is strongest
in the core and to the south and is small in the north.
The core, apparently containing two-thirds of the bolometric luminosity of
the inner 4" diameter area, may be explained by a thick, dusty torus near the
central AGN viewed at an angle of ~65 deg to its plane. There are, however,
detailed difficulties with existing models, especially the narrow east-west
width of the thin extended mid-infrared "tongue" to the north of the core. We
interpret the tongue as re-processed visual and ultraviolet radiation that is
strongly beamed and that originates in the AGN.Comment: 42 pages, 2 tables, 9 figures; Accepted for publication in A
Lifetime of 19Ne*(4.03 MeV)
The Doppler-shift attenuation method was applied to measure the lifetime of
the 4.03 MeV state in 19Ne. Utilizing a 3He-implanted Au foil as a target, the
state was populated using the 20Ne(3He,alpha)19Ne reaction in inverse
kinematics at a 20Ne beam energy of 34 MeV. De-excitation gamma rays were
detected in coincidence with alpha particles. At the 1 sigma level, the
lifetime was determined to be 11 +4, -3 fs and at the 95.45% confidence level
the lifetime is 11 +8, -7 fs.Comment: 6 pages, submitted to Phys. Rev.
Expressive and Instrumental Offending: Reconciling the Paradox of Specialisation and Versatility
Although previous research into specialisation has been dominated by the debate over the existence of specialisation versus versatility, it is suggested that research needs to move beyond the restrictions of this dispute. The current study explores the criminal careers of 200 offenders based on their criminal records, obtained from a police database in the North West of England, aiming to understand the patterns and nature of specialisation by determining the presence of differentiation within their general offending behaviours and examining whether the framework of Expressive and Instrumental offending styles can account for any specialised tendencies that emerge. Fifty-eight offences were subjected to Smallest Space Analysis. Results revealed that a model of criminal differentiation could be identified and that any specialisation is represented in terms of Expressive and Instrumental offending styles
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