Atelier "Étoiles à neutrons et leurs environnements" (MODE-SNR-PWN) 2018
11-13 juin 2018 Montpellier (France)
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Programme
Semaine
Lun. 11
Mar. 12
Mer. 13
Liste
lundi 11 juin 2018
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13:00
14:00
15:00
16:00
17:00
18:00
›13:00 (50min)
Accueil
13:00 - 13:50 (50min)
Accueil
Accueil des participants
›13:50 (10min)
Introduction
Y.Gallant
13:50 - 14:00 (10min)
Introduction
Y.Gallant
›14:00 (40min)
Computing accurate spectra of neutron stars for determining their parameters
F. Vincent (LUTH-Meudon)
14:00 - 14:40 (40min)
Computing accurate spectra of neutron stars for determining their parameters
F. Vincent (LUTH-Meudon)
›14:40 (25min)
Radio observations: LOFAR and NenuFAR
J.M. Griessmeier (LPC2E-Orléans)
14:40 - 15:05 (25min)
Radio observations: LOFAR and NenuFAR
J.M. Griessmeier (LPC2E-Orléans)
›15:05 (25min)
The infancy of supernova remnants - 3D long-time simulations of SN explosions
M.Gabler (MPA-Garching)
15:05 - 15:30 (25min)
The infancy of supernova remnants - 3D long-time simulations of SN explosions
M.Gabler (MPA-Garching)
›15:30 (25min)
Crust-core transition in magnetars
D. Chatterjee (LPC, Caen)
15:30 - 15:55 (25min)
Crust-core transition in magnetars
D. Chatterjee (LPC, Caen)
›15:55 (35min)
Pause café
15:55 - 16:30 (35min)
Pause café
›16:30 (25min)
HESS J1640/MSH 15-52
M.H. Grondin (CENBG-Bordeaux)- A. Mares (CENBG-Bordeaux)
16:30 - 16:55 (25min)
HESS J1640/MSH 15-52
M.H. Grondin (CENBG-Bordeaux)- A. Mares (CENBG-Bordeaux)
›16:55 (25min)
The VHE gamma-ray morphology of an asymmetric pulsar wind nebula
M. Tsirou (LUPM-Montpellier)
16:55 - 17:20 (25min)
The VHE gamma-ray morphology of an asymmetric pulsar wind nebula
M. Tsirou (LUPM-Montpellier)
›17:20 (25min)
Effects of ms pulsar winds on binary companions
A.Zilles (IAP-Paris)
17:20 - 17:45 (25min)
Effects of ms pulsar winds on binary companions
A.Zilles (IAP-Paris)
›17:45 (25min)
Blind source separation methods for extended sources viewed by high energy telescopes
F.Acero (AIM-Saclay)
17:45 - 18:10 (25min)
Blind source separation methods for extended sources viewed by high energy telescopes
F.Acero (AIM-Saclay)
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