144,812 research outputs found
Space power technology applied to the energy problem
A solution to the energy problem is suggested through the technology of photovoltaic electrolysis of water to generate hydrogen. Efficient solar devices are discussed in relation to available solar energy, and photovoltaic energy cost. It is concluded that photovoltaic electrolytic generation of hydrogen will be economically feasible in 1985
The galaxy halo formation rate
The rate at which galaxy halos form is thought to play a key role in
explaining many observable cosmological phenomena such as the initial epoch at
which luminous matter forms and the distribution of active galaxies. Here we
show how Press-Schechter theory can be used to provide a simple, completely
analytic model of the halo formation rate. This model shows good agreement with
both Monte-Carlo and N-body simulation results.Comment: 2 pages, 1 figure, to appear in proceedings of the Xth Recontres de
Blois, "The Birth of Galaxies," LaTeX style file include
X-ray reverberation in NLS1
Reverberation from scattering material around the black hole in active
galactic nuclei is expected to produce a characteristic signature in a Fourier
analysis of the time delays between directly-viewed continuum emission and the
scattered light. Narrow-line Seyfert 1 galaxies (NLS1) are highly variable at
X-ray energies, and are ideal candidates for the detection of X-ray
reverberation. We show new analysis of a small sample of NLS1 that clearly
shows the expected time-delay signature, providing strong evidence for the
existence of a high covering fraction of scattering and absorbing material a
few tens to hundreds of gravitational radii from the black hole. We also show
that an alternative interpretation of time delays in the NLS1 1H0707-495, as
arising about one gravitational radius from the black hole, is strongly
disfavoured in an analysis of the energy-dependence of the time delays.Comment: Published online in Proceedings of Science, "Narrow-line Seyfert 1
Galaxies and their place in the Universe", held in Milan, Italy April 4-6,
201
The hard X-ray spectrum of NGC 1365: scattered light, not black hole spin
Active Galactic Nuclei (AGN) show excess X-ray emission above 10 keV compared
with extrapolation of spectra from lower energies. Risaliti et al. have
recently attempted to model the hard X-ray excess in the type 1.8 AGN NGC 1365,
concluding that the hard excess most likely arises from Compton-scattered
reflection of X-rays from an inner accretion disk close to the black hole.
Their analysis disfavored a model in which the hard excess arises from a high
column density of circumnuclear gas partially covering a primary X-ray source,
despite such components being required in the NGC 1365 data below 10 keV. Using
a Monte Carlo radiative transfer approach, we demonstrate that this conclusion
is invalidated by (i) use of slab absorption models, which have unrealistic
transmission spectra for partial covering gas, (ii) neglect of the effect of
Compton scattering on transmitted spectra and (iii) inadequate modeling of the
spectrum of scattered X-rays. The scattered spectrum is geometry dependent and,
for high global covering factors, may dominate above 10 keV. We further show
that, in models of circumnuclear gas, the suppression of the observed hard
X-ray flux by reprocessing may be no larger than required by the `light
bending' model invoked for inner disk reflection, and the expected emission
line strengths lie within the observed range. We conclude that the
time-invariant `red wing' in AGN X-ray spectra is probably caused by continuum
transmitted through and scattered from circumnuclear gas, not by highly
redshifted line emission, and that measurement of black hole spin is not
possible.Comment: Revised version, accepted for publication by Ap.J. Letter
Cosmological evolution and hierarchical galaxy formation
We provide a new multi-waveband compilation of the data describing the
cosmological evolution of quasars, and discuss a model that attributes the
evolution to variation in the rate of merging between dark halos in a
hierarchical universe. We present a new Press-Schechter calculation of the
expected merger rate and show that this can reproduce the principal features of
the evolution. We also show that the evolution in the star-formation history of
the universe is well-described by this model.Comment: 4 pages, 1 figure. Presented at Xth Rencontres de Blois, "The Birth
of Galaxies", June 199
Appendix C: Faculty Publication
From the beginning the ILR faculty devoted much of its time and effort to the preparation and publication of works covering a wide range of subject matter within the industrial and labor relations field. Some of the faculty output addressed the interests of their scholarly colleagues and students but much was directed to practitioners and the general public as well
Chemotactic Turning Behaviour of Tubularia Spermatozoa
1. The movements of Tubularia spermatozoa in the vicinity of micropipettes filled with extracts of female hydranths, which chemotactically attract the spermatozoa, have been recorded by multiple-flash photomicrography.
2. When a spermatozoon turns in response to a chemotactic stimulus, the flagellum continues to beat, with a highly asymmetrical pattern of bending, during the turn.
3. The magnitude of the turn, particularly the duration of the period of asymmetrical beating, is variable, but each spermatozoon is only able to make turns in one direction, relative to its own body.
4. Most of the behaviour of these spermatozoa may be explained if the turning mechanism is activated when the spermatozoon detects a decreasing concentration of the chemotactant
New hyperthermal thermosetting heterocyclic polymers
Polyimidazopyrrolone polymers, formed by the condensation of aromatic dianhydrides with aromatic tetraamines in various solvents, form moldings that resist degradation in air and retain great strength at 400 to 700 degrees F. The resins have good insulating properties, are easy to mold, and make good protective coatings
The "backdoor pathway" of androgen synthesis in human male sexual development.
Mammalian sex determination (male versus female) is largely controlled by genes, whereas sex differentiation (development of reproductive structures) is largely controlled by hormones. Work in the 20th century indicated that female external anatomy was a "default" pathway of development not requiring steroids, whereas male genital development required testicular testosterone plus dihydrotestosterone (DHT) made in genital skin according to a "classic" pathway. Recent work added the description of an alternative "backdoor" pathway of androgen synthesis discovered in marsupials. Unique "backdoor steroids" are found in human hyperandrogenic disorders, and genetic disruption of the pathway causes disordered male sexual development, suggesting it plays an essential role. O'Shaughnessy and colleagues now show that the principal human backdoor androgen is androsterone and provide strong evidence that it derives from placental progesterone that is metabolized to androsterone in nontesticular tissues. These studies are essential to understanding human sexual development and its disorders
- …