From the 6 of 208 papers with an AI index.
129 citations
- Centre National de la Recherche ScientifiqueFR89 papers
- National Institute for AstrophysicsIT83 papers
- Max Planck Institute for Extraterrestrial PhysicsDE79 papers
- Sorbonne UniversitéFR73 papers
- Osservatorio Astronomico di PadovaIT71 papers
- University of BolognaIT70 papers
- University of CambridgeGB70 papers
- Max Planck Institute for AstronomyDE68 papers
- Brera Astronomical ObservatoryIT67 papers
- Osservatorio di Astrofisica e Scienza dello Spazio65 papers
- Université Paris-SaclayFR65 papers
- Institute for Space Astrophysics and PlanetologyIT64 papers
14 papers · 1 filter
A cosmic-ray loaded nascent outflow driven by a massive star cluster
Marianne Lemoine-Goumard, Lucia Härer, Lars Mohrmann +6
Cosmic rays are widely held to drive outflows from star-forming galaxies and profoundly influence galaxy evolution. Direct evidence for cosmic-ray carrying outflows is however lack…
The problem of escape: a missing bit in the theory of the origin of cosmic rays
P. Blasi, E. Amato
The escape of cosmic rays from their sources, as well as from the region surrounding a source, or from the galaxy hosting the sources, is a non-linear process that involves a compl…
Population synthesis of Galactic middle-aged pulsar wind nebulae I. Detection prospects for current and future instruments
A. De Sarkar, D. F. Torres, B. Olmi +2
Pulsar wind nebulae (PWNe) constitute the largest population of Galactic very-high-energy (VHE; GeV) -ray sources and are key laboratories for studying particle accel…
A thick-shell formalism for pulsar wind nebulae based on energy conservation
N. Bucciantini, B. Olmi
One of the most powerful approaches to model the structural and spectral evolution of wind bubbles, and pulsar wind nebulae in particular, is based on the one-zone thin-shell forma…
Old pulsar wind nebulae and the role of the thermal filaments
N. Bucciantini, Y. Batini, B. Olmi
Old pulsar wind nebulae are among the foremost galactic high-energy gamma-ray sources. However we still lack a robust approach to their modeling, especially in the light of forthco…
Suppressed diffusion and gamma-ray emission from the Cygnus bubble
Ben Li, Pasquale Blasi, Elena Amato
Recent gamma-ray observations indicate that star clusters can be efficient particle accelerators. In particular, LHAASO has detected diffuse gamma-ray emission from Cygnus OB2 exte…