Search Results - "Simonneau, E"
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Dark matter annihilation in the milky way galaxy: effects of baryonic compression
Published in Physical review letters (10-12-2004)“…If the dark matter (DM), which is considered to constitute most of the mass of galaxies, is made of supersymmetric particles, the central region of our Galaxy…”
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2
Thermodynamic Coefficients for Stellar Atmospheres and Plasma Spectroscopy
Published in The Astrophysical journal (20-04-2009)“…A new method to obtain the thermodynamic coefficients in an analytic and exact form for applications in radiative and convective transport in thermodynamic…”
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3
Method for Calculating the Opacity of the Atomic Lines in Stellar Atmospheres
Published in The Astrophysical journal (2009)“…A new approximate method for calculating the opacity of the atomic lines in the computation of stellar model atmospheres is presented. Transforming the sums in…”
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An improved version of the implicit integral method to solving radiative transfer problems
Published in Astrophysics (01-03-2012)“…Radiative transfer (RT) problems in which the source function includes a scattering-like integral are typical two-points boundary problems. Their solution via…”
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5
Inversion of stellar statistics equation for the Galactic bulge
Published in Monthly notices of the Royal Astronomical Society (01-04-2000)“…A method based on Lucy's iterative algorithm is developed to invert the equation of stellar statistics for the Galactic bulge and is then applied to the K-band…”
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6
A Forth-and-Back Implicit Λ-Iteration
Published in The Astrophysical journal (01-10-1997)Get full text
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7
An Implicit Integral Method to Solve Selected Radiative Transfer Problems. IV. The Case of Spherical Geometry
Published in The Astrophysical journal (01-11-1997)Get full text
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8
Multilevel Line Transfer with the Implicit Integral Method
Published in Astrophysics (01-10-2002)“…Once the need for an iterative procedure in order to solve the problem of the formation of spectral lines in the case of a model atom with many energy levels,…”
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9
How Far Do They Go? The Outer Structure of Galactic Dark Matter Halos
Published in The Astrophysical journal (10-07-2006)“…We study the density profiles of collapsed galaxy-size dark matter halos with masses 10 super(11) to 5 x 10 super(12) M sub( )focusing mostly on the halo outer…”
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10
Type I supernovae as distance indicators
Published in Astrophysics and space science (01-07-1989)Get full text
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11
Line transfer in supernovae envelopes by Sobolev's treatment
Published in Astrophysics and space science (01-07-1990)“…The effect of some physical parameters (the continuum opacity, the ratio of scattering over absorption, and the temperature profile) on the emergent intensity…”
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12
Iteration Profiles in Radiative Transfer Problems. I. From Vectorial to Scalar Coupling
Published in The Astrophysical journal (20-09-1995)Get full text
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13
Inversion of stellar statistics equation for the Galactic bulge
Published in Monthly notices of the Royal Astronomical Society (01-04-2000)Get full text
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14
An improved version of the Implicit Integral Method to solving radiative transfer problems
Published 10-10-2011“…Radiative transfer (RT) problems in which the source function includes a scattering-like integral are typical two-points boundary problems. Their solution via…”
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15
Radiative transfer models of dusty galaxian discs
Published in Monthly notices of the Royal Astronomical Society (01-10-1996)“…We present a set of face-on models of the radiative transfer of stellar light in exponential discs, taking into account absorption and multiple scattering…”
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16
Solution of line formation problem by use of iteration factors
Published in Journal of applied spectroscopy (01-09-1996)Get full text
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17
The intrinsic shape of bulges
Published 28-12-2010“…The structural parameters of a magnitude-limited sample of 148 unbarred S0-Sb galaxies were derived using the GASP2D algorithm and then analyzed to derive the…”
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18
Structural properties of spherical galaxies obeying the Sersic R^1/n law: a semi-analytical approach
Published 08-06-1999“…By considering that the distribution of measured light along any galactocentric radius of an elliptical galaxy can be well represented by a R^{1/n} Sersic law,…”
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Structural properties of disk galaxies. II. Intrinsic shape of bulges
Published 28-06-2010“…(Abridged) The structural parameters of a magnitude-limited sample of 148 unbarred S0-Sb galaxies were analyzed to derive the intrinsic shape of their bulges…”
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20
Structural properties of disk galaxies: The intrinsic equatorial ellipticity of bulges
Published 31-01-2008“…The structural parameters of a magnitude-limited sample of 148 unbarred S0-Sb galaxies were derived to study the correlations between bulge and disk parameters…”
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