2,244 research outputs found
Austin Powers meets Robin Hood: exploring texts through drama
Thesis (M.Ed.) University of Alaska Fairbanks, 2006This research project followed an ethnically and culturally diverse, sixth-grade classroom as they shared and constructed meaning from a selected text through a variety of drama activities. Unlike most studies on drama in the classroom, this research project examined the relationship between social construction of meaning through multiple literacies and the influence this has on student engagement. This study is centered in sociocultural theory, the central premise of which describes human thought as constituted by and originating from language-based social interactions with others. This research project also addressed the concept of multiple literacies and how it applied to the extension of communication choices beyond that of just language. It included drama, film, video, computer technology, visual arts, and music. As traditional forms of reading, writing, and communicating take on new literary forms, students need to be prepared and encouraged to critically think about the information they are exploring, especially in the area of media literacy. Through participant observation, field notes, fieldwork journal entries, audio and video recording, and interviews, I analyzed the students' social learning experiences, and their use of a variety of literacies to enhance and extend the traditional methods of reading, writing, speaking, and listening
High-fidelity view of the structure and fragmentation of the high-mass, filamentary IRDC G11.11-0.12
Star formation in molecular clouds is intimately linked to their internal
mass distribution. We present an unprecedentedly detailed analysis of the
column density structure of a high-mass, filamentary molecular cloud, namely
IRDC G11.11-0.12 (G11). We use two novel column density mapping techniques:
high-resolution (FWHM=2", or ~0.035 pc) dust extinction mapping in near- and
mid-infrared, and dust emission mapping with the Herschel satellite. These two
completely independent techniques yield a strikingly good agreement,
highlighting their complementarity and robustness. We first analyze the dense
gas mass fraction and linear mass density of G11. We show that G11 has a top
heavy mass distribution and has a linear mass density (M_l ~ 600 Msun pc^{-1})
that greatly exceeds the critical value of a self-gravitating, non-turbulent
cylinder. These properties make G11 analogous to the Orion A cloud, despite its
low star-forming activity. This suggests that the amount of dense gas in
molecular clouds is more closely connected to environmental parameters or
global processes than to the star-forming efficiency of the cloud. We then
examine hierarchical fragmentation in G11 over a wide range of size-scales and
densities. We show that at scales 0.5 pc > l > 8 pc, the fragmentation of G11
is in agreement with that of a self-gravitating cylinder. At scales smaller
than l < 0.5 pc, the results agree better with spherical Jeans' fragmentation.
One possible explanation for the change in fragmentation characteristics is the
size-scale-dependent collapse time-scale that results from the finite size of
real molecular clouds: at scales l < 0.5 pc, fragmentation becomes sufficiently
rapid to be unaffected by global instabilities.Comment: 8 pages, 8 figures, accepted to A&
Spin-Current Relaxation Time in Spin-Polarized Heisenberg Paramagnets
We study the spatial Fourier transform of the spin correlation function
G_q(t) in paramagnetic quantum crystals by direct simulation of a 1d lattice of
atoms interacting via a nearest-neighbor Heisenberg exchange Hamiltonian. Since
it is not practical to diagonalize the s=1/2 exchange Hamiltonian for a lattice
which is of sufficient size to study long-wavelength (hydrodynamic)
fluctuations, we instead study the s -> infinity limit and treat each spin as a
vector with a classical equation of motion. The simulations give a detailed
picture of the correlation function G_q(t) and its time derivatives. At high
polarization, there seems to be a hierarchy of frequency scales: the local
exchange frequency, a wavelength-independent relaxation rate 1/tau that
vanishes at large polarization P ->1, and a wavelength-dependent spin-wave
frequency proportional to q^2. This suggests a form for the correlation
function which modifies the spin diffusion coefficients obtained in a moments
calculation by Cowan and Mullin, who used a standard Gaussian ansatz for the
second derivative of the correlation function.Comment: 6 pages, 3 figure
Evidence that widespread star formation may be underway in G0.253+016, "The Brick"
Image cubes of differential column density as a function of dust temperature
are constructed for Galactic Centre molecular cloud G0.253+0.016 ("The Brick")
using the recently described PPMAP procedure. The input data consist of
continuum images from the Herschel Space Telescope in the wavelength range
70-500 m, supplemented by previously published interferometric data at 1.3
mm wavelength. While the bulk of the dust in the molecular cloud is consistent
with being heated externally by the local interstellar radiation field, our
image cube shows the presence, near one edge of the cloud, of a filamentary
structure whose temperature profile suggests internal heating. The structure
appears as a cool ( K) tadpole-like feature, pc in length, in
which is embedded a thin spine of much hotter ( 40-50 K) material. We
interpret these findings in terms of a cool filament whose hot central region
is undergoing gravitational collapse and fragmentation to form a line of
protostars. If confirmed, this would represent the first evidence of widespread
star formation having started within this cloud.Comment: 5 pages, 4 figures; accepted for publication in MNRAS Letter
Recommended from our members
Kinetics governing phase separation of nanostructured Sn_xGe_(1–x) alloys
We have studied the dynamic phenomenon of Sn_xGe_(1–x)/Ge phase separation during deposition by molecular beam epitaxy on Ge(001) substrates. Phase separation leads to the formation of direct band gap semiconductor nanowire arrays embedded in Ge oriented along the [001] growth direction. The effect of strain and composition on the periodicity were decoupled by growth on Ge(001) and partially relaxed Si_yGe_(1–y)/Ge(001) virtual substrates. The experimental results are compared with three linear instability models of strained film growth and find good agreement with only one of the models for phase separation during dynamic growth
Hierarchical fragmentation and collapse signatures in a high-mass starless region
Aims: Understanding the fragmentation and collapse properties of the dense
gas during the onset of high-mass star formation. Methods: We observed the
massive (~800M_sun) starless gas clump IRDC18310-4 with the Plateau de Bure
Interferometer (PdBI) at sub-arcsecond resolution in the 1.07mm continuum
andN2H+(3-2) line emission. Results: Zooming from a single-dish low-resolution
map to previous 3mm PdBI data, and now the new 1.07mm continuum observations,
the sub-structures hierarchically fragment on the increasingly smaller spatial
scales. While the fragment separations may still be roughly consistent with
pure thermal Jeans fragmentation, the derived core masses are almost two orders
of magnitude larger than the typical Jeans mass at the given densities and
temperatures. However, the data can be reconciled with models using
non-homogeneous initial density structures, turbulence and/or magnetic fields.
While most sub-cores remain (far-)infrared dark even at 70mum, we identify weak
70mum emission toward one core with a comparably low luminosity of ~16L_sun,
re-enforcing the general youth of the region. The spectral line data always
exhibit multiple spectral components toward each core with comparably small
line widths for the individual components (in the 0.3 to 1.0km/s regime). Based
on single-dish C18O(2-1) data we estimate a low virial-to-gas-mass ratio
<=0.25. We discuss that the likely origin of these spectral properties may be
the global collapse of the original gas clump that results in multiple spectral
components along each line of sight. Even within this dynamic picture the
individual collapsing gas cores appear to have very low levels of internal
turbulence.Comment: 8 pages, 4 figures, A&A in pres
On the temperature structure of the Galactic Centre cloud G0.253+0.016
We present a series of smoothed particle hydrodynamical models of
G0.253+0.016 (also known as 'The Brick'), a very dense molecular cloud that
lies close to the Galactic Centre. We explore how its gas and dust temperatures
react as we vary the strength of both the interstellar radiation field (ISRF)
and the cosmic ray ionisation rate (CRIR). As the physical extent of
G0.253+0.016 along our line-of-sight is unknown, we consider two possibilities:
one in which the longest axis is that measured in the plane of the sky (9.4 pc
in length), and one in which it is along the line of sight, in which case we
take it to be 17 pc. To recover the observed gas and dust temperatures, we find
find that the ISRF must be around 1000 times the solar neighbourhood value, and
the CRIR must be roughly 1E-14 /s, regardless of the geometries studied. For
such high values of the CRIR, we find that cooling in the cloud's interior is
dominated by neutral oxygen, in contrast to standard molecular clouds, which at
the same densities are mainly cooled via CO. Our results suggest that the
conditions near G0.253+0.016 are more extreme than those generally accepted for
the inner 500 pc of the galaxy.Comment: 6 pages, 4 figures, 1 table, accepted for publication in ApJ Letter
Void-mediated formation of Sn quantum dots in a Si matrix
Atomic scale analysis of Sn quantum dots (QDs) formed during the molecular beam-epitaxy (MBE) growth of Sn_xSi_(1−x) (0.05 ⩽ x ⩽ 0.1) multilayers in a Si matrix revealed a void-mediated formation mechanism. Voids below the Si surface are induced by the lattice mismatch strain between Sn_xSi_(1−x) layers and Si, taking on their equilibrium tetrakaidecahedron shape. The diffusion of Sn atoms into these voids leads to an initial rapid coarsening of quantum dots during annealing. Since this formation process is not restricted to Sn, a method to grow QDs may be developed by controlling the formation of voids and the diffusion of materials into these voids during MBE growth
- …