8,378 research outputs found
Dust properties along anomalous extinction sightlines. II. Studying extinction curves with dust models
The large majority of extinction sight lines in our Galaxy obey a simple
relation depending on one parameter, the total-to-selective extinction
coefficient, Rv. Different values of Rv are able to match the whole extinction
curve through different environments so characterizing normal extinction
curves. In this paper more than sixty curves with large ultraviolet deviations
from their best-fit one parameter curve are analyzed. These curves are fitted
with dust models to shed light into the properties of the grains, the processes
affecting them, and their relations with the environmental characteristics. The
extinction curve models are reckoned by following recent prescriptions on grain
size distributions able to describe one parameter curves for Rv values from 3.1
to 5.5. Such models, here extended down to Rv=2.0, allow us to compare the
resulting properties of our deviating curves with the same as normal curves in
a self-consistent framework, and thus to recover the relative trends overcoming
the modeling uncertainties. Such curves represent the larger and homogeneous
sample of anomalous curves studied so far with dust models. Results show that
the ultraviolet deviations are driven by a larger amount of small grains than
predicted for lines of sight where extinction depends on one parameter only.
Moreover, the dust-to-gas ratios of anomalous curves are lower than the same
values for no deviating lines of sight. Shocks and grain-grain collisions
should both destroy dust grains, so reducing the amount of the dust trapped
into the grains, and modify the size distribution of the dust, so increasing
the small-to-large grain size ratio. Therefore, the extinction properties
derived should arise along sight lines where shocks and high velocity flows
perturb the physical state of the interstellar medium living their signature on
the dust properties. (Abridged version)Comment: 31 pages,12 figures; accepted for publication in A&
Projectile compositions and modal frequencies on the chemistry of micrometeoroids LDEF experiment
The Chemistry of Micrometeoroids Experiment (LDEF instrument A0187-1) exposed witness plates of high-purity gold (greater than 99.99 percent Au) and commercial aluminum (greater than 99 percent Al) with the objective of analyzing the residues of cosmic-dust and orbital-debris particles associated with hypervelocity impact craters. The gold substrates were located approximately 8 deg off LDEF's trailing edge (Bay A03), while the aluminum surfaces resided in Bay A11, approximately 52 deg from LDEF's leading edge. SEM-EDX techniques were employed to analyze the residues associated with 199 impacts on the gold and 415 impacts on the aluminum surfaces. The residues that could be analyzed represent natural or man-made materials. The natural particles dominate at all particle sizes less than 5 micron. It is possible to subdivide both particle populations into subclasses. Chondritic compositions dominate the natural impactors (71 percent), followed by monomineralic, mafic-silicate compositions (26 percent), and by Fe-Ni rich sulfides (approximately 3 percent). Approximately 30 percent of all craters on the gold collectors were caused by man-made debris such as aluminum, paint flakes, and other disintegrated, structural and electronic components. Equations-of-state and associated calculations of shock stresses for typical LDEF impacts into the gold and aluminum substrates suggest that substantial vaporization may have occurred during many of the impacts and is the reason why approximately 50 percent of all craters did not contain sufficient residue to permit analysis by the SEM-EDX technique. After converting the crater diameters into projectile sizes using encounter speeds typical for the trailing-edge and forward-facing (Row 11) directions, and accounting for normalized exposure conditions of the CME collectors, we derived the absolute and relative fluxes of specific projectile classes. The natural impactors encounter all LDEF pointing directions with comparable, modal frequencies suggesting compositional (and dynamic) homogeneity of the interplanetary-dust environment in near-Earth orbit
Astrophysical science metrics for next-generation gravitational-wave detectors
The second generation of gravitational-wave detectors are being built and
tuned all over the world. The detection of signals from binary black holes is
beginning to fulfill the promise of gravitational-wave astronomy. In this work,
we examine several possible configurations for third-generation laser
interferometers in existing km-scale facilities. We propose a set of
astrophysically motivated metrics to evaluate detector performance. We measure
the impact of detector design choices against these metrics, providing a
quantitative cost-benefit analyses of the resulting scientific payoffs
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