THE BROADBAND EMISSION FROM SUPERNOVA REMNANT RX J0852.0-4622
Journal Article
·
· Astrophysical Journal
- Department of Physics, Yunnan University, Kunming (China)
We study the nonthermal emission from SNR RX J0852.0-4622 based on a self-consistent kinetic method that describes the nonlinear shock acceleration of cosmic rays in supernova remnants (SNRs). In this method, the spectrum of accelerated protons in the SNR can be self-consistently calculated, where a proton's maximum momentum is determined by equating the SNR's age with the acceleration time of the proton. At the same time, the spectrum of accelerated electrons is similar to the proton's spectrum if the electron's momentum is much less than the electron's maximum momentum (p{sub e,max}), which is estimated by equating the synchrotron loss time to the acceleration time of the electrons, but the cutoff shapes around p{sub e,max} are assumed to be exponential. Using the accelerated particle's spectra, we calculate nonthermal photon spectra for different values of some main model parameters such as the SNR's age, an injection parameter, and a background magnetic field. Moreover, we study possible (hadronic or leptonic) origins of very high energy (VHE) {gamma}-ray emission from SNR RX J0852.0-4622. Our results indicate that a hadronic origin of VHE {gamma}-rays from SNR RX J0852.0-4622 seems to be more reasonable although a leptonic origin cannot be ruled out. We suggest that the observations of Fermi LAT for this remnant will help us find the evidence to determine the main emission mechanism.
- OSTI ID:
- 21464846
- Journal Information:
- Astrophysical Journal, Journal Name: Astrophysical Journal Journal Issue: 1 Vol. 721; ISSN ASJOAB; ISSN 0004-637X
- Country of Publication:
- United States
- Language:
- English
Similar Records
Gamma-Ray Observations of the Supernova Remnant RX J0852.0-4622 with the Fermi LAT
NON-THERMAL X-RAY EMISSION FROM THE NORTHWESTERN RIM OF THE GALACTIC SUPERNOVA REMNANT G266.2-1.2 (RX J0852.0-4622)
MULTIBAND NONTHERMAL EMISSION FROM THREE TeV SHELL-TYPE SUPERNOVA REMNANTS
Journal Article
·
Mon Dec 12 19:00:00 EST 2011
· Astrophysical Journal Letters
·
OSTI ID:1032745
NON-THERMAL X-RAY EMISSION FROM THE NORTHWESTERN RIM OF THE GALACTIC SUPERNOVA REMNANT G266.2-1.2 (RX J0852.0-4622)
Journal Article
·
Fri Oct 01 00:00:00 EDT 2010
· Astrophysical Journal
·
OSTI ID:21464763
MULTIBAND NONTHERMAL EMISSION FROM THREE TeV SHELL-TYPE SUPERNOVA REMNANTS
Journal Article
·
Sun Apr 10 00:00:00 EDT 2011
· Astrophysical Journal
·
OSTI ID:21574769
Related Subjects
73 NUCLEAR PHYSICS AND RADIATION PHYSICS
79 ASTRONOMY AND ASTROPHYSICS
ACCELERATION
BARYONS
BOSONS
COSMIC RADIATION
COSMIC RADIO SOURCES
ELECTROMAGNETIC RADIATION
ELECTRONS
ELEMENTARY PARTICLES
EMISSION
FERMIONS
GAMMA RADIATION
HADRONS
IONIZING RADIATIONS
LEPTONS
MAGNETIC FIELDS
MASSLESS PARTICLES
NUCLEONS
PHOTONS
PROTON SPECTRA
PROTONS
RADIATIONS
SPECTRA
SUPERNOVA REMNANTS
79 ASTRONOMY AND ASTROPHYSICS
ACCELERATION
BARYONS
BOSONS
COSMIC RADIATION
COSMIC RADIO SOURCES
ELECTROMAGNETIC RADIATION
ELECTRONS
ELEMENTARY PARTICLES
EMISSION
FERMIONS
GAMMA RADIATION
HADRONS
IONIZING RADIATIONS
LEPTONS
MAGNETIC FIELDS
MASSLESS PARTICLES
NUCLEONS
PHOTONS
PROTON SPECTRA
PROTONS
RADIATIONS
SPECTRA
SUPERNOVA REMNANTS