Seminar

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18 February 2020

Flow in the vicinity of compact object

Le 11 mars 2016 De 10h30 à 12h00 Zakaria Meliani Observatoire de Paris-Meudon Accretion disks play an important role in the evolution of their relativistic inner compact objects. The emergence of a new generation of interferometers will allow resolving these accretion disks...

18 February 2020

The MUSE Instrument for Lyman-alpha Haloes Detection

Le 4 mars 2016 De 10h30 à 12h00 Jean-Baptiste COURBOT ICube - Université de StrasbourgThe Multi-Unit Spectroscopic Explorer (MUSE) instrument, located at the VLT, allows the investigation of a wide spectral range across a 1x1 arcmin sky region. In particular, its spectral...

18 February 2020

Dark Stars

Le 19 février 2016 De 10h30 à 12h00 Douglas SPOLYAR Stockholm UniversityDark Stars (DS) are stellar objects made (almost entirely) of ordinary atomic material but powered by the heat from Dark Matter (DM) annihilation (rather than by fusion). Weakly Interacting Massive...

18 February 2020

M4AST : On-line tool for spectral modeling of asteroids

Le 29 janvier 2016 De 10h30 à 12h00 Mirel BIRLAN IMCCE, Observatoire de Paris M4AST (Modelling for asteroids) is a tool devoted to model and interpret spectra data in the visible and near-infrared of asteroids. It is composed by an asteroid spectral database and a set of...

18 February 2020

First glimpse into Gaia’s astrometry – a progress report

Le 11 décembre 2015 De 10h30 à 12h00 Ulrich BASTIAN ARI, Heidelberg According to the official plan, the first astrometric data releases from Gaia are expected by mid 2016 (positions only) and mid 2017 (incl. parallaxes and proper motions). This is the time needed to collect...

18 February 2020

Planck et les grandes structures

Le 27 novembre 2015 De 10h30 à 12h00 Hervé DOLE Institut d'Astrophysique Spatiale, Orsay Le satellite Planck, pierre angulaire de l’ESA dédiée à la cosmologie et lancé en 2009, a observé la totalité du ciel pendant près de 2 ans et demi, et mesuré le fond diffus...

18 February 2020

Magnetism in massive stars

Le 13 novembre 2015 De 10h30 à 12h00 Coralie NEINER Observatoire de Paris I will present the latest observational results obtained on the magnetic fields of massive stars thanks mainly to large spectropolarimetric programs. I will discuss the origin of these magnetic fields,...