Amanote Research

Amanote Research

    RegisterSign In

Understanding the Diffuse Gamma Ray Emission of the Milky Way - From Supernova Remnants to Dark Matter

Matica Srpska Journal for Natural Sciences
doi 10.2298/zmspn1937017p
Full Text
Open PDF
Abstract

Available in full text

Date

January 1, 2019

Authors
Jovana PetrovicTijana ProdanovicMilos Kovacevic
Publisher

National Library of Serbia


Related search

Dark Matter in the Milky Way

2016English

Observed and Expected 1–30 Tev Gamma-Ray Emission From Geminga and Tycho's Supernova Remnants

International Journal of Modern Physics A
NuclearMolecular Physics,High Energy PhysicsAtomicAstrophysicsAstronomyOptics
2005English

CO Emission From Supernova Remnants

Astrophysical Journal
AstrophysicsAstronomyPlanetary ScienceSpace
1977English

Constraints on Cosmic-Ray Origin From TeV Gamma-Ray Observations of Supernova Remnants

1997English

Gamma-Ray Emission Expected From Kepler's Supernova Remnant

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2006English

Multiwavelength Analysis of Annihilating Dark Matter as the Origin of the Gamma-Ray Emission From M31

Physical Review D
AstronomyPhysics
2018English

Radio Emission From Shell-Type Supernova Remnants

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2006English

Radio Emission From 16 Possible Supernova Remnants

Australian Journal of Physics
1969English

Current and Future Constraints on Dark Matter From Prompt and Inverse-Compton Photon Emission in the Isotropic Diffuse Gamma-Ray Background

Physical Review D
2012English

Amanote Research

Note-taking for researchers

Follow Amanote

© 2025 Amaplex Software S.P.R.L. All rights reserved.

Privacy PolicyRefund Policy