16,610 research outputs found
New Insights on Interstellar Gas-Phase Iron
In this paper, we report on the gas-phase abundance of singly-ionized iron
(Fe II) for 51 lines of sight, using data from the Far Ultraviolet
Spectroscopic Explorer (FUSE). Fe II column densities are derived by measuring
the equivalent widths of several ultraviolet absorption lines and subsequently
fitting those to a curve of growth. Our derivation of Fe II column densities
and abundances creates the largest sample of iron abundances in moderately- to
highly-reddened lines of sight explored with FUSE, lines of sight that are on
average more reddened than lines of sight in previous Copernicus studies. We
present three major results. First, we observe the well-established correlation
between iron depletion and and also find trends between iron depletion
and other line of sight parameters (e.g. f(H_2), E_(B-V), and A_V), and examine
the significance of these trends. Of note, a few of our lines of sight probe
larger densities than previously explored and we do not see significantly
enhanced depletion effects. Second, we present two detections of an extremely
weak Fe II line at 1901.773 A in the archival STIS spectra of two lines of
sight (HD 24534 and HD 93222). We compare these detections to the column
densities derived through FUSE spectra and comment on the line's f-value and
utility for future studies of Fe II. Lastly, we present strong anecdotal
evidence that the Fe II f-values derived empirically through FUSE data are more
accurate than previous values that have been theoretically calculated, with the
probable exception of f_1112.Comment: Accepted for publication in ApJ, 669, 378; see ApJ version for small
updates. 53 total pages (preprint format), 7 tables, 11 figure
The Abundance of Interstellar Fluorine and Its Implications
We report results from a survey of neutral fluorine (F I) in the interstellar
medium. Data from the Far Ultraviolet Spectroscopic Explorer (FUSE) were used
to analyze 26 lines of sight lying both in the galactic disk and halo,
including lines to Wolf-Rayet stars and through known supernova remnants. The
equivalent widths of fluorine resonance lines at 951.871 A and 954.827 A were
measured or assigned upper limits and combined with a nitrogen curve of growth
to obtain F I column densities. These column densities were then used to
calculate fluorine depletions. Comparisons are made to the previous study of F
I by Federman et al. (2005) and implications for F I formation and depletion
are discussed.Comment: 32 pages, 10 figures, Accepted to Ap
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Affect's Effects: Considering Art-activism and the 2001 Crisis in Argentina
Anxious of straying too far from traditional rational actor models and an assiduous positivism, social movement scholars have displayed a persistent tendency to overlook the specificities of visual tools and aesthetic experience in claim-making and political protest. Often, as a direct consequence, the possibilities for mobilization and the matrices within which action takes place are described and understood in ways that are oversimplified, even distorted. Notably, small steps have been taken to overcome these distortions by building in a theory of affect that reserves a crucial space for the extra-discursive in the study of contentious politics. Extending some of these insights, this article reveals how an affect-informed approach can be particularly illuminating in studies of art-activism. It takes stencil protests from the aftermath of the 2001 crisis in Argentina as a case in point, discussing affects and their effects on porteño street artists. In so doing, it strengthens the case for greater incorporation of affect as a tool for understanding in literatures that deal with questions of framing, art-activism and the possibilities for social change
Why Trade Associations Matter: Exploring Function, Meaning, and Influence
We explore the organizational characteristics of trade associations (TAs) and suggest theoretical approaches for undertaking research into or involving TAs in management and organization studies. Through emphasizing the role of TAs within and between industries and at the interface of business and society, we consider how TAs generate meaning and influence
Abundances and Physical Conditions in the Interstellar Gas toward HD 192 639
We present a study of the abundances and physical conditions in the
interstellar gas toward the heavily reddened star HD 192639 [E_(B-V) = 0.64],
based on analysis of FUSE and HST/STIS spectra covering the range from 912 to
1361 A. This work constitutes a survey of the analyses that can be performed to
study the interstellar gas when combining data from different instruments.
Low-velocity (-18 to -8 km/s) components are seen primarily for various neutral
and singly ionized species such as C I, O I, S I, Mg II, Cl I, Cl II, Mn II, Fe
II and Cu II. Numerous lines of H2 are present in the FUSE spectra, with a
kinetic temperature for the lowest rotational levels T_(01) = (90 +/- 10) K.
Analysis of the C I fine-structure excitation implies an average local density
of hydrogen n_H = (16 +/- 3) cm^-3. The average electron density, derived from
five neutral/first ion pairs under the assumption of photoionization
equilibrium, is n_e = (0.11 +/- 0.02) cm^-3. The relatively complex component
structure seen in high-resolution spectra of K I and Na I, the relatively low
average density, and the measured depletions all suggest that the line of sight
contains a number of diffuse clouds, rather than a single dense, translucent
cloud. Comparisons of the fractions of Cl in Cl I and of hydrogen in molecular
form suggest a higher molecular fraction, in the region(s) where H2 is present,
than that derived considering the average line of sight. In general, such
comparisons may allow the identification and characterization of translucent
portions of such complex lines of sight. The combined data also show
high-velocity components near -80 km/s for various species which appear to be
predominantly ionized, and may be due to a radiative shock. A brief overview of
the conditions in this gas will be given.Comment: 37 pages, accepted for publication in Ap
Navigating the Terrain of Third Space: Tensions with/in Relationships in School-University Partnerships
Using theoretical conceptions of third space and hybrid teacher education, we engaged in a collaborative self-study of our practices as university-based teacher educators working in student teaching partnership settings. We sought to understand the ways in which the hybrid teacher educator fosters and mediates relationships to work towards a collective third space. In this article, we describe the nature of relationships in our work, the tensions wrought by complexities of these relationships, and ways we negotiated tensions in order to foster relationships that productively mediated processes of teacher education. In addition, we propose a framework for moving beyond traditional notions of oppositional triadic relationships of student teacher, mentor teacher, and supervisor in recognition of complex social interactions in the third space
Precision determination of absolute neutron flux
A technique for establishing the total neutron rate of a highly-collimated
monochromatic cold neutron beam was demonstrated using a method of an
alpha-gamma counter. The method involves only the counting of measured rates
and is independent of neutron cross sections, decay chain branching ratios, and
neutron beam energy. For the measurement, a target of 10B-enriched boron
carbide totally absorbed the neutrons in a monochromatic beam, and the rate of
absorbed neutrons was determined by counting 478keV gamma rays from neutron
capture on 10B with calibrated high-purity germanium detectors. A second
measurement based on Bragg diffraction from a perfect silicon crystal was
performed to determine the mean de Broglie wavelength of the beam to a
precision of 0.024 %. With these measurements, the detection efficiency of a
neutron monitor based on neutron absorption on 6Li was determined to an overall
uncertainty of 0.058 %. We discuss the principle of the alpha-gamma method and
present details of how the measurement was performed including the systematic
effects. We also describe how this method may be used for applications in
neutron dosimetry and metrology, fundamental neutron physics, and neutron cross
section measurements.Comment: 44 page
Gender Attitudes and Fertility Aspirations among Young Men in Five High Fertility East African Countries
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/97275/1/j.1728-4465.2013.00341.x.pd
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