FERMI LAT DISCOVERY OF EXTENDED GAMMA-RAY EMISSION IN THE DIRECTION OF SUPERNOVA REMNANT W51C
Top Cited Papers
- 27 October 2009
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 706 (1), L1-L6
- https://doi.org/10.1088/0004-637x/706/1/l1
Abstract
No abstract availableKeywords
This publication has 24 references indexed in Scilit:
- MILAGRO OBSERVATIONS OF MULTI-TeV EMISSION FROM GALACTIC SOURCES IN THE FERMI BRIGHT SOURCE LISTThe Astrophysical Journal, 2009
- FERMI/LARGE AREA TELESCOPE BRIGHT GAMMA-RAY SOURCE LISTThe Astrophysical Journal Supplement Series, 2009
- THE LARGE AREA TELESCOPE ON THEFERMI GAMMA-RAY SPACE TELESCOPEMISSIONThe Astrophysical Journal, 2009
- High energy astrophysics with ground-based gamma ray detectorsReports on Progress in Physics, 2008
- The Third EGRET Catalog of High‐Energy Gamma‐Ray SourcesThe Astrophysical Journal Supplement Series, 1999
- Radio to Gamma‐Ray Emission from Shell‐Type Supernova Remnants: Predictions from Nonlinear Shock Acceleration ModelsThe Astrophysical Journal, 1999
- The W51 Giant Molecular CloudThe Astronomical Journal, 1998
- EGRET Observations of Radio-bright Supernova RemnantsThe Astrophysical Journal, 1996
- Particle acceleration at astrophysical shocks: A theory of cosmic ray originPhysics Reports, 1987
- Proper motions and distances of H2O maser sources. II - W51 MAINThe Astrophysical Journal, 1981