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