Atelier « Étoiles à neutrons et leurs environnements » (MODE-SNR-PWN 2019)

A Review of the Spider Pulsar Population

René Breton

X-ray observations of Spiders

Mallory Roberts

Nancay Radio Telescope discovery of the eclipsing black widow pulsar PSR J2055+3829

Lucas Guillemot

Coffee break

The future of MODE SNR-PWN workshops

Plenary discussion

Lunch

X-raying nearby thermal and non-thermal remnants : The case of Magellanic supernova remnants, superbubbles, and pulsar wind nebulae

Pierre Maggi

The population of PWNe seen by HESS and their Galactic environments

Yves Gallant

A deep look at the HESS J1825-137 pulsar wind nebula with H.E.S.S. and Fermi-LAT

Sami Caroff

Efficient particle acceleration from HESS J1640.6-4633 and the PeVatron candidate HESS J1641.0-4619

Arnaud Marès

Is G150.3+4.5 old or one of the closest GeV gamma-ray SNRs ?

Justine Devin

Coffee break

Towards a better understanding of dense matter with gravitational waves

Jérôme Margueron

Constraints on Dense Matter Equation of State from GW170817: Possibility of Different Families of Compact Stars

Prasanta Char

The stability properties of differentially rotating neutron stars

Pawel Szewczyk

Neutron star properties from an extended linear sigma model

János Takátsy

Planning