2,135 research outputs found
Photovoltaic effect in ferroelectric ceramics
The ceramic structure was simulated in a form that is more tractable to correlation between experiment and theory. Single crystals (of barium titanate) were fabricated in a simple corrugated structure in which the pedestals of the corrugation simulated the grain while the intervening cuts could be filled with materials simulating the grain boundaries. The observed photovoltages were extremely small (100 mv)
Chemical evolution in the early phases of massive star formation II: Deuteration
The chemical evolution in high-mass star-forming regions is still poorly
constrained. Studying the evolution of deuterated molecules allows to
differentiate between subsequent stages of high-mass star formation regions due
to the strong temperature dependence of deuterium isotopic fractionation. We
observed a sample of 59 sources including 19 infrared dark clouds, 20 high-mass
protostellar objects, 11 hot molecular cores and 9 ultra-compact HII regions in
the (3-2) transitions of the four deuterated molecules, DCN, DNC, DCO+ and N2D+
as well as their non-deuterated counterpart. The overall detection fraction of
DCN, DNC and DCO+ is high and exceeds 50% for most of the stages. N2D+ was only
detected in a few infrared dark clouds and high-mass protostellar objects. It
can be related to problems in the bandpass at the frequency of the transition
and to low abundances in the more evolved, warmer stages. We find median D/H
ratios of ~0.02 for DCN, ~0.005 for DNC, ~0.0025 for DCO+ and ~0.02 for N2D+.
While the D/H ratios of DNC, DCO+ and N2D+ decrease with time, DCN/HCN peaks at
the hot molecular core stage. We only found weak correlations of the D/H ratios
for N2D+ with the luminosity of the central source and the FWHM of the line,
and no correlation with the H2 column density. In combination with a previously
observed set of 14 other molecules (Paper I) we fitted the calculated column
densities with an elaborate 1D physico-chemical model with time-dependent
D-chemistry including ortho- and para-H2 states. Good overall fits to the
observed data have been obtained the model. It is one of the first times that
observations and modeling have been combined to derive chemically based
best-fit models for the evolution of high-mass star formation including
deuteration.Comment: 26 pages, 16 figures, accepted at A&
Chemical evolution in the early phases of massive star formation. I
Understanding the chemical evolution of young (high-mass) star-forming
regions is a central topic in star formation research. Chemistry is employed as
a unique tool 1) to investigate the underlying physical processes and 2) to
characterize the evolution of the chemical composition. We observed a sample of
59 high-mass star-forming regions at different evolutionary stages varying from
the early starless phase of infrared dark clouds to high-mass protostellar
objects to hot molecular cores and, finally, ultra-compact HII regions at 1mm
and 3mm with the IRAM 30m telescope. We determined their large-scale chemical
abundances and found that the chemical composition evolves along with the
evolutionary stages. On average, the molecular abundances increase with time.
We modeled the chemical evolution, using a 1D physical model where density and
temperature vary from stage to stage coupled with an advanced gas-grain
chemical model and derived the best-fit chi^2 values of all relevant
parameters. A satisfying overall agreement between observed and modeled column
densities for most of the molecules was obtained. With the best-fit model we
also derived a chemical age for each stage, which gives the timescales for the
transformation between two consecutive stages. The best-fit chemical ages are
~10,000 years for the IRDC stage, ~60,000 years for the HMPO stage, ~40,000
years for the HMC stage, and ~10,000 years for the UCHII stage. The total
chemical timescale for the entire evolutionary sequence of the high-mass star
formation process is on the order of 10^5 years, which is consistent with
theoretical estimates. Furthermore, based on the approach of a multiple-line
survey of unresolved data, we were able to constrain an intuitive and
reasonable physical and chemical model. The results of this study can be used
as chemical templates for the different evolutionary stages in high-mass star
formation.Comment: 31 pages, 11 figures, 21 tables, accepted by A&A; typos adde
Long-term Variability of HCO Masers in Star-forming Regions
We present results of a multi-epoch monitoring program on variability of
6cm formaldehyde (HCO) masers in the massive star forming region
NGC7538IRS1 from 2008 to 2015 conducted with the GBT, WSRT, and
VLA. We found that the similar variability behaviors of the two formaldehyde
maser velocity components in NGC7538IRS1 (which was pointed out by
Araya and collaborators in 2007) have continued. The possibility that the
variability is caused by changes in the maser amplification path in regions
with similar morphology and kinematics is discussed. We also observed
12.2GHz methanol and 22.2GHz water masers toward
NGC7538IRS1. The brightest maser components of CHOH and HO
species show a decrease in flux density as a function of time. The brightest
HCO maser component also shows a decrease in flux density and has a similar
LSR velocity to the brightest HO and 12.2GHz CHOH masers. The line
parameters of radio recombination lines and the 20.17 and 20.97GHz CHOH
transitions in NGC7538IRS1 are also reported. In addition, we
observed five other 6cm formaldehyde maser regions. We found no evidence of
significant variability of the 6cm masers in these regions with respect to
previous observations, the only possible exception being the maser in
G29.960.02. All six sources were also observed in the HCO
isotopologue transition of the 6cm HCO line; HCO absorption
was detected in five of the sources. Estimated column density ratios
[HCO]/[HCO] are reported.Comment: 29 pages, 9 figure
AVIAN USE OF ROADSIDE HABITAT IN THE SOUTHERN DRIFT PLAINS OF NORTH DAKOTA AND IMPLICATIONS FOR CATTAIL (\u3ci\u3eTYPHA\u3c/i\u3e SPP.) MANAGEMENT
We determined avian use of roadside rights-of-way to develop proper management strategies for the manipulation of roadside cattail. Cattail management is a technique used to reduce nesting and roosting habitat for problematic blackbird species, which might feed on sunflower crops in the vicinity of cattail-dominated wetlands. Thirty quarter sections (1 quarter section ≈ 64.75 ha) located in the Southern Drift Plains of North Dakota served as our study units. Roadside habitat along two 0.5 mile (-0.8 km) transects bordering these quarter sections was surveyed to assess avian use. Additionally, nest surveys were , conducted to provide an index of breeding bird use of this roadside habitat. Finally, roadside habitat was surveyed for a number of different habitat variables. We found 49 different species during the surveys. Of the 2,529 birds found in this habitat, 1,479 (41.5%) were blackbirds. Blackbirds were also the primary nesting birds, contributing to 89% of the active nests found in roadside habitat. In terms of avian use and nesting, blackbirds, especially redwings, were the dominant bird species using roadside cattail. With proper management of roadside habitat, potential effects on non-blackbirds can be minimized, and nesting habitat for blackbirds can be reduced. Our data Indicate that a loss in nesting habitat will likely result in fewer blackbirds and a subsequent reduction in sunflower damage
Non-Target Hazard Assessment of Using DRC-1339 Avicide to Manage Blackbirds in Sunflower
Terrestrial hazard assessments were conducted for the spring blackbird baiting program to protect sunflower crops. Risk Assessment methodology proposed by the Ecological Committee on FIFRA Risk Assessment Methods (ECOFRAM) and the method currently used by the U.S. Environmental Protection Agency (LD50s/ft2) were compared for their predictive strengths and for the ease of adapting the assessment to site specific conditions. While the ECOFRAM and LD50s/ft2 methods identified the same groups of organisms as being at risk, the flexibility of the ECOFRAM methodology allowed more latitude in adapting the assessment to unique behaviors of individual species. These risk assessment approaches indicate that blackbird baiting with DRC-1339 presents acute hazards to select nontarget birds like western meadowlarks and mourning doves but few hazards to most mammals or small granivorous birds like sparrows and finches. However, field experiments indicate that the mitigation measures currently employed in the baiting program, minimize the nontarget hazards
Dogs increase recovery of passerine carcasses in dense vegetation
Wildlife managers use carcass searches to assess mortality resulting from biological (e.g., diseases) and physical (e.g., structure collisions) sources. Carcass searches may occur over large areas and need to be completed rapidly because of scavenging and decomposition. However, small carcasses are often missed when dense vegetation is searched. We placed carcasses of house sparrows (Passer domesticus) in dense cover of residual and newly grown vegetation and compared searching efficiency of humans and canines. Dogs received no special training in searching for passerine carcasses. In 36 trials conducted in 5 x 40-m plots, human searchers found 45% (SD=19) of the carcasses compared to 92% (SD=13) for dogs (P=0.005). The ratio of recovered to missed carcasses was approximately 12:l for dogs and 1 :I for humans. The improvement in searching efficiency using dogs was similar (P=0.58) between residual cover (searched in April) and new growth cover (searched in August). A greater rate of searching efficiency is obtained per unit of time by using dogs. Greater efficiency improves quantitative and qualitative assessments of avian mortality in the field
Influence of the Dufour effect on convection in binary gas mixtures
Linear and nonlinear properties of convection in binary fluid layers heated
from below are investigated, in particular for gas parameters. A Galerkin
approximation for realistic boundary conditions that describes stationary and
oscillatory convection in the form of straight parallel rolls is used to
determine the influence of the Dufour effect on the bifurcation behaviour of
convective flow intensity, vertical heat current, and concentration mixing. The
Dufour--induced changes in the bifurcation topology and the existence regimes
of stationary and traveling wave convection are elucidated. To check the
validity of the Galerkin results we compare with finite--difference numerical
simulations of the full hydrodynamical field equations. Furthermore, we report
on the scaling behaviour of linear properties of the stationary instability.Comment: 14 pages and 10 figures as uuencoded Postscript file (using uufiles
Influence of the Soret effect on convection of binary fluids
Convection in horizontal layers of binary fluids heated from below and in
particular the influence of the Soret effect on the bifurcation properties of
extended stationary and traveling patterns that occur for negative Soret
coupling is investigated theoretically. The fixed points corresponding to these
two convection structures are determined for realistic boundary conditions with
a many mode Galerkin scheme for temperature and concentration and an accurate
one mode truncation of the velocity field. This solution procedure yields the
stable and unstable solutions for all stationary and traveling patterns so that
complete phase diagrams for the different convection types in typical binary
liquid mixtures can easily be computed. Also the transition from weakly to
strongly nonlinear states can be analyzed in detail. An investigation of the
concentration current and of the relevance of its constituents shows the way
for a simplification of the mode representation of temperature and
concentration field as well as for an analytically manageable few mode
description.Comment: 30 pages, 12 figure
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