A population synthesis study with a hybrid TIDE+L dynamical model predicts that the Cherenkov Telescope Array Observatory will detect roughly ten times more Galactic pulsar wind nebulae than are currently known in TeV gamma rays.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
fields
astro-ph.HE 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
SN 2023dbc is a moderately energetic, highly obscured Type Ib supernova with estimated kinetic energy 4.1e51 erg, ejecta mass 2.3 solar masses, and nickel mass 0.038 solar masses, consistent with an aspherical explosion and partial fallback from a 15 solar mass binary progenitor that retained helium
citing papers explorer
-
Population synthesis of Galactic middle-aged pulsar wind nebulae I. Detection prospects for current and future instruments
A population synthesis study with a hybrid TIDE+L dynamical model predicts that the Cherenkov Telescope Array Observatory will detect roughly ten times more Galactic pulsar wind nebulae than are currently known in TeV gamma rays.
-
SN 2023dbc in M108: Optical and Near-Infrared Observations of a Highly-Obscured, Moderately Energetic Stripped-Envelope Supernova
SN 2023dbc is a moderately energetic, highly obscured Type Ib supernova with estimated kinetic energy 4.1e51 erg, ejecta mass 2.3 solar masses, and nickel mass 0.038 solar masses, consistent with an aspherical explosion and partial fallback from a 15 solar mass binary progenitor that retained helium