Multi-messenger model for the starburst galaxy M82

Abstract

In this paper, a consistent model of the multifrequency emission of the starburst galaxy M82, from radio to gamma-rays is presented and discussed. Predictions for observations with Fermi, MAGIC II/VERITAS and CTA telescopes are made. The model is also used to self-consistenty compute the (all flavors) emission of neutrinos resulting from this starburst galaxy, what can be used in considerations of the diffuse contributions of such objects.

Accepted for publication in The Astrophysical Journal

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Cited by in corpus (60)

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• Detection of Gamma-Ray Emission from the Starburst Galaxies M82 and NGC 253 with the Large Area Telescope on Fermi
• On The GeV & TeV Detections of the Starburst Galaxies M82 & NGC 253
• Time-Integrated Searches for Point-like Sources of Neutrinos with the 40-String IceCube Detector
• Ultra-High-Energy Cosmic Rays
• Cosmic Neutrino Pevatrons: A Brand New Pathway to Astronomy, Astrophysics, and Particle Physics
• Winds, Clumps, and Interacting Cosmic Rays in M82
• The Equipartition Magnetic Field Formula in Starburst Galaxies: Accounting for Pionic Secondaries and Strong Energy Losses
• Diffuse PeV neutrinos from EeV cosmic ray sources: semi-relativistic hypernova remnants in star-forming galaxies
• Cosmic ray transport and radiative processes in nuclei of starburst galaxies
• Gamma-rays from molecular clouds illuminated by accumulated diffusive protons. II: interacting supernova remnants
• What IceCube data tell us about neutrino emission from star-forming galaxies (so far)
• A propeller scenario for the gamma-ray emission of low-mass X-ray binaries: The case of XSS J12270-4859
• Acceleration of ultrahigh-energy cosmic rays in starburst superwinds
• The Star-Forming Galaxy Contribution to the Cosmic MeV and GeV Gamma-Ray Background
• Contribution of starburst nuclei to the diffuse gamma-ray and neutrino flux
• Diffuse Hard X-ray Emission in Starburst Galaxies as Synchrotron from Very High Energy Electrons
• High Energy Emission from the Starburst Galaxy NGC253
• ASTRI Mini-Array Core Science at the Observatorio del Teide
• Simulating radio synchrotron emission in star-forming galaxies: small-scale magnetic dynamo and the origin of the far infrared-radio correlation
• Are Starburst Galaxies Proton Calorimeters?
• Equipartition and Cosmic Ray Energy Densities in Central Molecular Zones of Starbursts
• Cosmic rays and non-thermal emission in simulated galaxies. II. $\gamma$-ray maps, spectra and the far infrared-$\gamma$-ray relation
• The Radio-Gamma Correlation In Starburst Galaxies
• Interpreting the Low Frequency Radio Spectra of Starburst Galaxies: A Pudding of Strömgren Spheres
• SOFIA Far Infrared Imaging Polarimetry of M82 and NGC 253: Exploring the Super-Galactic Wind
• Cosmic rays in galaxies: a probe of star formation
• Molecular environment, reverberation, and radiation from the pulsar wind nebula in CTA 1
• Gamma-ray signatures of cosmic ray acceleration, propagation, and confinement in the era of CTA
• High Energy Gamma-ray Absorption and Cascade Emission in Nearby Starburst Galaxies
• Exploring the physics behind the non-thermal emission from star-forming galaxies detected in gamma rays
• Inverse Compton Contribution to the Star-Forming Extragalactic Gamma-Ray Background
• Estimates of relativistic electron and proton energy densities in starburst galactic nuclei from radio measurements
• X-Ray Emission from Star-Forming Galaxies - Signatures of Cosmic Rays and Magnetic Fields
• Starburst and post-starburst high-redshift protogalaxies: The feedback impact of high energy cosmic rays
• Tracing star formation with non-thermal radio emission
• Interstellar gamma-ray emission from cosmic rays in star-forming galaxies
• Building up the spectrum of cosmic-rays in star-forming regions
• Cosmic Ray Sampling of a Clumpy Interstellar Medium
• Extragalactic Observatory Science with the ASTRI Mini-Array at the Observatorio del Teide
• Gamma-ray emission from spectrally resolved cosmic rays in galaxies
• Production of secondary particles in heavy nuclei interactions in supernova remnants
• Ultrahigh-Energy Cosmic Ray Composition from the Distribution of Arrival Directions
• Exploring the superwind mechanism for generating ultrahigh-energy cosmic rays using large-scale modeling of starbursts
• Synchrotron and Compton Spectra from a Steady-State Electron Distribution
• Cosmic-ray transport and gamma-ray emission in M31
• Energetic Particles in Halos of Star Forming Galaxies
• CONGRuENTS (COsmic-ray, Neutrino, Gamma-ray and Radio Non-Thermal Spectra). I. A predictive model for galactic non-thermal emission
• From 10 Kelvin to 10 TeraKelvin: Insights on the Interaction Between Cosmic Rays and Gas in Starbursts
• Highlight Talk: Recent Results from VERITAS
• Evidence for UHECR origin in starburst galaxies
• On the possible correlation of Galactic VHE source locations and enhancements of the surface density in the Galactic plane
• Olber's Paradox for Superluminal Neutrinos: Constraining Extreme Neutrino Speeds at TeV-ZeV Energies with the Diffuse Neutrino Background
• Energetic Particles in the Central Starburst, Disc, and Halo of NGC253
• Bayesian approach to equipartition estimation of magnetic field strength
• Nonthermal Emission from Star-Forming Galaxies
• Non-thermal emission in the central starburst region of M82
• Echoes of the past: ultra-high energy cosmic rays accelerated by radio galaxies, scattered by starburst galaxies