67,700 research outputs found
Education for citizenship: the Joseph Rowntree Charitable Trust and the educational settlement movement
No abstract available
SINFONI's take on Star Formation, Molecular Gas, and Black Hole Masses in AGN
We present some preliminary (half-way) results on our adaptive optics
spectroscopic survey of AGN at spatial scales down to 0.085arcsec. Most of the
data were obtained with SINFONI which provides integral field capability at a
spectral resolution of R~4000. The themes on which we focus in this
contribution are: star formation around the AGN, the properties of the
molecular gas and its relation to the torus, and the mass of the black hole.Comment: 5 pages, 2 figures. To appear in Science Perspectives for 3D
Spectroscopy. ESO Astrophysics Symposia. Ed by M. Kissler-Patig, M. Roth and
J. Wals
The Low Surface Brightness Extent of the Fornax Cluster
We have used a large format CCD camera to survey the nearby Fornax cluster
and its immediate environment for low luminosity low surface brightness
galaxies. Recent observations indicate that these are the most dark matter
dominated galaxies known and so they are likely to be a good tracer of the dark
matter in clusters. We have identified large numbers of these galaxies
consistent with a steep faint end slope of the luminosity function (alpha~ -2)
down to MB ~ -12. These galaxies contribute almost the same amount to the total
cluster light as the brighter galaxies and they have a spatial extent that is
some four times larger. They satisfy two of the important predictions of N-body
hierarchical simulations of structure formation using dark halos. The
luminosity (mass ?) function is steep and the mass distribution is more
extended than that defined by the brighter galaxies. We also find a large
concentration of low surface brightness galaxies around the nearby galaxy
NGC1291.Comment: 16 pages, 6 figure
Establishing an analogue population for the most distant galaxies
Lyman break analogues (LBAs) are local galaxies selected to match a more
distant (usually z~3) galaxy population in luminosity, UV-spectral slope and
physical characteristics, and so provide an accessible laboratory for exploring
their properties. However, as the Lyman break technique is extended to higher
redshifts, it has become clear that the Lyman break galaxies (LBGs) at z~3 are
more massive, luminous, redder, more extended and at higher metallicities than
their z~5 counterparts. Thus extrapolations from the existing LBA samples
(which match z=3 properties) have limited value for characterising z>5
galaxies, or inferring properties unobservable at high redshift. We present a
new pilot sample of twenty-one compact star forming galaxies in the local
(0.05<z<0.25) Universe, which are tuned to match the luminosities and star
formation volume densities observed in z>~5 LBGs. Analysis of optical emission
line indices suggests that these sources have typical metallicities of a few
tenths Solar (again, consistent with the distant population). We also present
radio continuum observations of a subset of this sample (13 sources) and
determine that their radio fluxes are consistent with those inferred from the
ultraviolet, precluding the presence of a heavily obscured AGN or significant
dusty star formation.Comment: 13 pages, MNRAS accepte
Study of the Barringer Refractor Plate Correlation Spectrometer as a remote sensing instrument
Barringer refractor plate correlation spectrometer as remote sensing instrument of pollutant gases in atmospher
Non-singlet coefficient functions for charged-current deep-inelastic scattering to the third order in QCD
We have calculated the coefficient functions for the structure functions F_2,
F_L and F_3 in nu-nubar charged-current deep-inelastic scattering (DIS) at the
third order in the strong coupling alpha_s, thus completing the description of
unpolarized inclusive W^(+-) exchange DIS to this order of massless
perturbative QCD. In this brief note, our new results are presented in terms of
compact approximate expressions that are sufficiently accurate for
phenomenological analyses. For the benefit of such analyses we also collect, in
a unified notation, the corresponding lower-order contributions and the flavour
non-singlet coefficient functions for nu+nubar charged-current DIS. The
behaviour of all six third-order coefficient functions at small Bjorken-x is
briefly discussed.Comment: 6 pages, LaTeX (PoS style), 1 eps-figure. Fortran files of the main
results available with the source. To appear in the proceedings of `DIS
2016', DESY, Hamburg (Germany), April 201
Varieties of liberalism: Anglo-Saxon capitalism in crisis?
‘Global financial crisis’ is an inaccurate description of the current upheaval in the world’s financial markets. The initial banking crisis did not affect all countries to the same degree. Notably, while the US and UK banking systems
were badly hit, those of the other two major Anglo-Saxon economies, Canada and Australia, remain largely unscathed and have even gained in terms of global market share. The national business systems and comparative corporate governance literatures underscore the similarities among these four ‘liberal market economies’ (LMEs) and would predict similar trajectories. This paper investigates the reasons behind the differing performance of the Anglo-Saxon
banking systems, which defy a verdict of failure of the LME variety of capitalism as such
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