227,730 research outputs found
Approximate likelihood inference in generalized linear latent variable models based on integral dimension reduction
Latent variable models represent a useful tool for the analysis of complex
data when the constructs of interest are not observable. A problem related to
these models is that the integrals involved in the likelihood function cannot
be solved analytically. We propose a computational approach, referred to as
Dimension Reduction Method (DRM), that consists of a dimension reduction of the
multidimensional integral that makes the computation feasible in situations in
which the quadrature based methods are not applicable. We discuss the
advantages of DRM compared with other existing approximation procedures in
terms of both computational feasibility of the method and asymptotic properties
of the resulting estimators.Comment: 28 pages, 3 figures, 7 table
The Effects of Galaxy Shape and Rotation on the X-ray Haloes of Early-Type Galaxies
We present a detailed diagnostic study of the observed temperatures of the
hot X-ray coronae of early-type galaxies. By extending the investigation
carried out in Pellegrini (2011) with spherical models, we focus on the
dependence of the energy budget and temperature of the hot gas on the galaxy
structure and internal stellar kinematics. By solving the Jeans equations we
construct realistic axisymmetric three-component galaxy models (stars, dark
matter halo, central black hole) with different degrees of flattening and
rotational support. The kinematical fields are projected along different lines
of sight, and the aperture velocity dispersion is computed within a fraction of
the circularized effective radius. The model parameters are chosen so that the
models resemble real ETGs and lie on the Faber-Jackson and Size-Luminosity
relations. For these models we compute T_* (the stellar heating contribution to
the gas injection temperature) and T_gm (the temperature equivalent of the
energy required for the gas escape). In particular, different degrees of
thermalisation of the ordered rotational field of the galaxy are considered. We
find that T_* and T_gm can vary only mildly due to a pure change of shape.
Galaxy rotation instead, when not thermalised, can lead to a large decrease of
T_*; this effect can be larger in flatter galaxies that can be more
rotationally supported. Recent temperature measurements T_x, obtained with
Chandra, are larger than, but close to, the T_* values of the models, and show
a possible trend for a lower T_x in flatter and more rotationally supported
galaxies; this trend can be explained by the lack of thermalisation of the
whole stellar kinetic energy. Flat and rotating galaxies also show lower L_x
values, and then a lower gas content, but this is unlikely to be due to the
small variation of T_gm found here for them.Comment: 16 pages, 7 figures, accepted for publication in MNRA
The "Canone Inverso": when tobacco was not so bad. A Look Back at the Primordial Debate on the tobacco effects in the Occupational Medicine
AIM: The article provides an overview on the beginning and evolutions of medical observations on tobacco induced diseases between Eighteenth and Nineteenth century.
METHODS: By searching for historical medical literature, first studies on tobacco-induced diseases focused on production risks rather than on adverse effects that the use of tobacco has for the human health.
RESULTS: The approach induced first eighteenth-century authors to define this substance as a non-pathogenic and, consequently, not to consider tobacco factories dangerous for health workers. In those years, tobacco was employed in therapy as a stimulant treatment and it was considered harmless and even healthy and preventive of several acute diseases.
CONCLUSIONS: Authors will show that studies on pathogenic effects of smoking will only start around late nineteenth century, when the idea of the healthiness of tobacco industry was already supported
The 'Foce' monumental cemetery in Sanremo: mirror of the city as outstanding tourist destination during the Belle Epoque (1880-1915)
The monumental cemetery of Sanremo, was founded in 1838 and now counts about 2000 graves, one third of which belongs to foreigners, evidences of the city as outstanding tourist destination. The city with a good climate was also choosen for the recovery from the disease of chest by many people, even by Maria Alessandrovna, Csarina of Russia.
Many important people came to Sanremo from all over the world and sometimes here passed by and were buried: people like the painter Edward Lear, the anatomist Arthur Hill Hassal, Lady Caroline Giffard Phillipson, Prussian nobles, a good number of Russian aristocrats, and many others..
Compactifying the image of the Abel map
Let be the Abel map of multidegree
of a singular curve of genus . We describe the closure of inside Caporaso's compactified Jacobian
for irreducible curves, curves of compact type and binary curves
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