MODE-SNR-PWN Workshop

Program of the workshop

Marianne Lemoine — 2010-11-23T14:18:39Z

Monday 15th November:

José Pons, Magneto-thermal evolution of neutron stars
Thierry Foglizzo, Supernovae explosions
Michael Gabler, Magneto-elastic oscillations and the damping of crustal shear modes in magnetars
Mikhail Gusakov, Decoupling of superfluid and normal modes in pulsating neutron stars
Andrey Chugunov, Oscillations of superfluid neutron stars
Michal Bejger, Creation of millisecond pulsars via disk accretion and the EOS of dense matter
Petr Shternin, Cooling of neutron star crust in quasi-persistent X-ray transients: Evidence for additional heating
Morgane Fortin, Thermalization time and specific heat of neutron stars crust
Jason Hessels, Charting The transient radio sky on sub-second time scales with LOFAR
Pasquale Blasi, Cosmic-ray leptons and hadrons from SNRs
Jean Heyvaerts, Torsional oscillations of new-born quark stars as sources of long gamma ray bursts
Chiara Ceccobello, Montecarlo simulations of emerging spectra in strong magnetic field atmospheres of neutron stars
Daniele Vigano, Neutron Star magnetosphere static solutions
Luca Bonanno, Magnetic fields generated by r-modes in accreting quark stars

Tuesday 16th November:

Wednesday 17th November:

1. Session SN:

Alessandro Drago, Rapidly rotating SN and GRB progenitors: magnetic fields formation and quark deconfinement
Irina Sagert, Quark matter in neutron stars and core-collapse supernovae
Anthea Fantina, Impact of electro-weak processes in type II supernovae collapse
Francesca Gulminelli, Statistical description of complex nuclear phases in supernovae and proto-neutron stars
Micaela Oertel, An extended equation of state for core collapse simulations
Silvano Bonazzola, 6-D neutrino transport
Chatterjee Debarati, Suprathermal viscosity of superfluid neutron star matter and emission of gravitational waves

2. Session SNR:

Yves Gallant, (V)HE gamma-ray sources and particle acceleration in the Galaxy
Matthieu Renaud, Towards a complete sensus of the youngest Galactic SNRs
Jean Ballet, Possible origins of the spectrum of Fermi SNRs
Gilles Maurin, Geometry of acceleration in the bipolar remnant of SN1006 with XMM-Newton
Jeremie Mehault, [SNR W41 as seen by HESS]
François Brun, [SNR W49B as seen by HESS]

SNR-PWN Workshop in Montpellier (May 2010)

Marianne Lemoine — 2010-06-26T13:21:08Z

Jean Ballet, X-ray Observations of Supernova Remnants
Eveline Helder, Cosmic-Ray Acceleration in Supernova Remnants
Alexandre Marcowith, Young Supernova Remnants and Cosmic-Ray Physics
Matthieu Renaud, Cas A: latest INTEGRAL results and Multiwavelength Observations
Marianne Lemoine-Goumard, Supernova Remnants with Fermi after 1.5 year of Observations
Melitta Naumann-Godo, SN1006 as seen with HESS
Marie-Helene Grondin, Pulsar Wind Nebulae as seen with Fermi-LAT
Yves Gallant, Very high energy emitting PWNe
Fabio Mattana, Vela-X and other young PWNe observed with INTEGRAL

Previous workshops

Marianne Lemoine — 2010-06-26T13:17:21Z

SNR/PWN Workshop in Montpellier (May 2010):

The detailed program as well as the presentations from this workshop can be found at this address

MODE 2009 Workshop in Meudon (November 2009):

The detailed program as well as the presentations from this workshop can be found at this address

General Information

Marianne Lemoine — 2010-06-26T10:03:58Z

General map

Bordeaux map

University map

Transports

- From the airport to Bordeaux down town (most hotels)
You can take a bus "JET'BUS" (7 euros / pers) every 45 minutes from 7:45 to 22:45 - Departure from airport Hall B. Stop at "Office de Tourisme", 1-3 allée de Tourny, from which Hotels are less than 10 min by walk. Time table for this shuttle are available on this page.
Or you can go by taxi, it will cost about 40-50 euros. You can find some additional information on this page

- From the train station to the hotels You can take the tram line C headed to "Les Aubiers" and get off at stop "Place de la Bourse" around which most hotels are located

Accomodations

We encouraged you to book your hotels as soon as possible. You can find some informations in the Hotels section. Most hotels are located in Bordeaux down town (except two in Talence).

Meeting place

The meeting will take place in Bordeaux University (Talence). To go there from downtown take the tram line B headed to "Pessac" (or "Bougnard") and get off at the stop named "Forum". From there you can walk up to Le Haut Carre where the meeting will be. We'll have lunch there too.

Here is a more detailed map of Bordeaux University focused on the "Haut Carre"

Social dinner

On Tuesday night, we will have a social dinner in Bordeaux.

Warning

Please book your hotel and fill the registration form as soon as possible.

For more informations you can have a look at the dedicated sections or send an email to : lemoine@cenbg.in2p3.fr

List of participants

Isabelle Moreau — 2010-06-25T13:47:28Z

- List of participants

Isabelle Moreau — 2010-06-25T12:27:43Z

MODE-SNR-PWN Meeting

Bordeaux - 15- 17 November 2010

Thank you for your registration.

DO NOT FORGET TO RESERVE YOUR ROOM BY PHONE OR EMAIL DIRECTLY TO YOUR HOTEL.

You will receive an email of confirmation.

MODE-SNR-PWN Workshop in Bordeaux
15-17 November 2010

Isabelle Moreau — 2010-06-25T12:18:08Z

The workshop MODE-SNR-PWN will bring together three different communities interested in the physics of neutron stars: the neutron star observers, the supernova remnants and pulsar wind nebulae observers and the theoreticians (microphysics and macroscopic modelisation). It is supported by the GDR PCHE and CompStar-ESF.

Scientific summary

Over the last decade an enormous amount of new information about neutron stars has been accumulated by the satellites like XMM-NEWTON, CHANDRA, INTEGRAL, FERMI, and the earth laboratories, in particular the different radio-telescopes, but also the HESS observatory. Moreover, very interesting informations are expected to shed light on compact stars in the near future thanks to the gravitational-wave detectors like VIRGO and LIGO. Various new phenomenons related for instance to the enormous magnetic fields (Flares and QPO), to the reheating of the crust or to pulsar wind nebulae in supernovae remnants have been observed. A thorough understanding of all these phenomena requires to bring together leading and promising young researchers from all the fields. Important issues to address include: What can we learn from these new observations about neutron star structure and the radiation mechanism? Which models shall be developed to analyze the new data? What would be key observations for the future?

Meeting program

The workshop shall help the three communities to exchange with each other as well as discussing internal advanced issues. To that end the program will contain parallel specialized sessions as well as plenary sessions with reviews and a round table to help the discussion among the communities. All sessions will be held in the same place (Le Haut Carré, Talence) to allow everyone to circulate from one session to another. The sessions will be arranged in such a way to create “focus sessions” around certain topics, among them:

Radio timing, rotating neutron stars,
General relativity and neutron star modelisation,
Equation of state,
Observation at different wave lengths,
Emission processes and supernovae,
Supernovae remnants and pulsar wind nebulae.

Organizing committee

Marianne Lemoine-Goumard (CENBG, Bordeaux), Jérôme Margueron (IPN Orsay), Micaela Oertel (LUTH, Meudon), Matthieu Renaud (LPTA, Montpellier), Gilles Theureau (GEPI, Observatoire de Paris).

Credits

Isabelle Moreau — 2010-06-25T09:10:42Z

Ce site a été réalisé par le Centre d'Etudes Nucléaires de Bordeaux Gradignan, dans le cadre du projet d'harmonisation des webs du CNRS, en se basant sur dif férentes sources citées ci-après.

Ce site utilise :

Le kit graphique et html fournit par les équipes de la Direction des Systèmes d'Information et de la Délégation à l'Information Scientifique et Technique du CNRS, basé sur une charte conçue et développée selon une création originale et d'après des principes de systèmes graphiques créés par le studio "Eliane Design" ( http://www.elianedesign.com ).

Le système de publication dynamique SPIP : http://www.spip.net/

Les menus déroulants en CSS dynamique utilisent HOVER - V 1.00 2003 - Peter Nederlo f : http://www.xs4all.nl/ peterned/

Si vous souhaitez des renseignements sur l'utilisation de ces sources pour votre site Web, vous pouvez contacter notre Webmaster .

Crédit photos :

Les images utilisées pour la réalisation de ce site Web du CNRS proviennent des archives du CNRS "Diffusion Vidéothèque Photothèque" ainsi que de la photothèque de l'IN2P3. Elles sont la propriété du CNRS. Toute copie, totale ou partielle, ne peut se faire sans l'accord du CNRS.

Mentions légales

Isabelle Moreau — 2010-06-25T09:10:36Z

Centre d'Etudes Nucléaires de Bordeaux Gradignan Chemin du Solarium 33175 Gradignan Cedex

Tél. : +33 (0) 5 57 12 08 00 Fax. : +33 (0) 5 57 12 08 01

Directeur de la publication : Bernard Haas

Hébergeur : CENBG Chemin du Solarium 33175 Gradignan Cedex

Protection des informations nominatives

Ce site Web, qui comporte des informations nominatives concernant notamment les personnels du CNRS et de ses partenaires, a fait l'objet d'une déclaration auprès de la Cnil (avis n° 650931).Conformément à la loi n° 78-17 du 6 janvier 1978, relative à l'Informatique, aux fichiers et aux Libertés (articles 34, 36, 38, 39, 40), vous disposez d'un droit d'accès, de rectification et de suppression des données vous concernant, en ligne sur ce site.

Pour exercer ce droit, vous pouvez vous adresser au Webmaster

Conditions d'utilisation

Clause de non-responsabilité : La responsabilité du CNRS ne peut, en aucune manière, être engagée quant au contenu des informations figurant sur ce site ou aux conséquences pouvant résulter de leur utilisation ou interprétation.

Propriété intellectuelle

Le site du CNRS est une oeuvre de création, propriété exclusive du CNRS, protégé par la législation française et internationale sur le droit de la propriété intellectuelle. Aucune reproduction ou représentation ne peut être réalisée en contravention avec les droits du CNRS issus de la législation susvisée.

Liens hypertextes

La mise en place de liens hypertextes par des tiers vers des pages ou des documents diffusés sur le site du CNRS, est autorisée sous réserve que les liens ne contreviennent pas aux intérêts du CNRS, et, qu'ils garantissent la possibilité pour l'utilisateur d'identifier l'origine et l'auteur du document.