XMM-Newton observations of HESS J1813-178 reveal a composite Supernova remnant

2006/11/20 by S. Funk, J. A. Hinton, Y. Moriguchi +15 · 2 citations
Physics and Astronomy · #Astronomy #Astrophysical Phenomena and Observations #Astrophysics #Astrophysics and Cosmic Phenomena #Geology #Physics #Pulsars and Gravitational Waves Research #Supernova #Supernova remnant #astro-ph

paper · pdf · doi:10.1051/0004-6361:20066779

published as Astron.Astrophys.470:249-258,2007 · Submitted to A&A

arxiv created 2006/11/20 · openalex publication_date 2007/05/16 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Aims.We present X-ray and 12CO() observations of the very-high-energy (VHE) γ-ray source HESS J1813-178 with the aim of understanding the origin of the γ-ray emission.

Citations

• GLIMPSE. I. AnSIRTFLegacy Project to Map the Inner Galaxy
• SwiftXRT Follow‐up Observations of TeV Sources of the HESS Inner Galaxy Survey
• H I in the Galaxy
• New Catalogs of Compact Radio Sources in the Galactic Plane
• Ultracompact HII regions: the impact of newly formed massive stars on their environment
• Very high energy gamma rays from the composite SNR G 0.9+0.1
• Discovery of Very High Energy Gamma Rays Associated with an X-ray Binary
• The Evolution and Structure of Pulsar Wind Nebulae
• A New Population of Very High Energy Gamma-Ray Sources in the Milky Way

Cited by

• MASSIVE STARS IN THE Cl 1813-178 CLUSTER: AN EPISODE OF MASSIVE STAR FORMATION IN THE W33 COMPLEX
• Discovery of an X-ray nebula around PSR J1718-3825 and implications for the nature of the γ-ray source HESS J1718–385