XMM-Newton observations of Sagittarius A East
arXiv:astro-ph/0312541 · doi:10.1111/j.1365-2966.2004.07571.x
Abstract
We present an analysis of a recent XMM-Newton observation of Sgr A East, a supernova remnant located close to the Galactic Centre. Very high quality X-ray spectra reveal many emission lines from highly ionized atoms consistent with a multi-temperature thin thermal plasma in ionization equilibrium. We use a two-temperature model to fit the spectra and derive temperatures of 1 keV and 4 keV. There is significant concentration of iron towards the centre of the X-ray source such that the iron abundance varies from ~4 times solar in the core down to ~0.5 solar in the outer regions, which contrasts with the rather uniform distribution of other metals such as sulfur, argon and calcium, which have abundances in the range 1--3. The derived total energy, mass, and the abundance pattern are consistent with a single supernova event, either of type-Ia or type-II origin, involving a relatively low-mass progenitor star. A weak 6.4-keV neutral iron fluorescence line is also detected, the illumination source most likely being Sgr A East itself. The morphology and spectral characteristics of Sgr A East show no clear linkage to putative past activity in Sgr A*.
arXiv comment12 pages, 8 figures, to appear in MNRAS, figures with full resolution available at http://www.star.le.ac.uk/~mas/research/paper/#Sakano2003mnras
References in corpus (28)
- The European Photon Imaging Camera on XMM-Newton: The MOS Cameras
- Chandra X-ray Spectroscopic Imaging of Sgr A* and the Central Parsec of the Galaxy
- Rapid X-ray flaring from the direction of the supermassive black hole at the Galactic Centre
- Stellar Dynamics in the Galactic centre: Proper Motions and Anisotropy
- Nucleosynthesis in Type Ia Supernovae
- Nucleosynthesis and Mixing in Cassiopeia A
- Nucleosynthesis in Type II Supernovae
- XMM-Newton observation of the brightest X-ray flare detected so far from SgrA*
- A Chandra Study of Sgr A East: A Supernova Remnant Regulating The Activity Of Our Galactic Center?
- A Deep Chandra Catalog of X-ray Point Sources toward the Galactic Center
- ASCA X-ray source catalogue in the Galactic Center region
- A New X-Ray Flare from the Galactic Nucleus Detected with the XMM-Newton Photon Imaging Cameras
- XMM-Newton observation of the Tycho Supernova Remnant
- Stellar Iron Abundances at the Galactic Center
- ASCA Observations of the Sgr B2 Cloud: An X-Ray Reflection Nebula
- On the Origin of the Iron K Line in the Spectrum of the Galactic X-ray Background
- Chandra Observations of Diffuse X-Rays from the Sagittarius B2 Cloud
- High-resolution Observations of OH(1720 MHz) Masers Toward the Galactic Center
- The X-ray Iron Emission from Tycho's Supernova Remnant
- ASCA Discovery of Diffuse 6.4 keV Emission Near the Sgr C Complex: A New X-ray Reflection Nebula
- The Galactic Center: An Interacting System of Unusual Sources
- A Kinship between the EGRET SNR's and Sgr A East
- Hyperstrong Radio-Wave Scattering in the Galactic Center. I. A Survey for Extragalactic Sources Seen Through the Galactic Center
- The discovery of a new non-thermal X-ray filament near the Galactic Centre
- A catalogue of soft X-ray sources in the galactic center region
- Unusual Properties of X-Ray Emission near the Galactic Center
- A Self-Consistent Model for the Broad-band Spectrum of Sgr A East at the Galactic Center
- A Model of the EGRET Source at the Galactic Center: Inverse Compton Scattering Within Sgr A East and its Halo
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- The Galactic Center Massive Black Hole and Nuclear Star Cluster
- The Relation Between Optical Extinction and Hydrogen Column Density in the Galaxy
- Stellar Processes Near the Massive Black Hole in the Galactic Center
- Line derived infrared extinction towards the Galactic Center
- Iron and Nickel Line Diagnostics for the Galactic Center Diffuse Emission
- Discovery of a 3.5 keV line in the Galactic Center and a Critical Look at the Origin of the Line Across Astronomical Targets
- Chemical Abundances of Luminous Cool Stars in the Galactic Center from High-Resolution Infrared Spectroscopy
- The chemical abundances in the Galactic Centre from the atmospheres of Red Supergiants
- Traces of past activity in the Galactic Centre
- A Persistent High-Energy Flux from the Heart of the Milky Way : Integral's view of the Galactic Center
- Interstellar gas within pc of Sgr A
- Concurrent X-ray, near-infrared, sub-millimeter, and GeV gamma-ray observations of Sgr A*
- A Catalog of Diffuse X-ray-Emitting Features within 20 pc of Sgr A*: Twenty Pulsar Wind Nebulae?
- Asymmetric Type-Ia supernova origin of W49B as revealed from spatially resolved X-ray spectroscopic study
- A Candidate Neutron Star Associated with Galactic Center Supernova Remnant Sagittarius A East
- Discoveries of Diffuse Iron Line Sources from the Sgr B Region
- The X-ray outburst of the Galactic Centre magnetar SGR J1745-2900 during the first 1.5 year
- Unusual X-ray transients in the Galactic Centre
- Unbound Debris Streams and Remnants Resulting From the Tidal Disruptions of Stars by Supermassive Black Holes
- Diffuse X-Ray Sky in the Galactic Center
- Progenitor Mass Distribution of Core-Collapse Supernova Remnants in Our Galaxy and Magellanic Clouds based on Elemental Abundances
- The Metal-enriched Thermal Composite Supernova Remnant Kesteven 41 (G337.8-0.1) in a Molecular Environment
- The Sgr B2 X-ray Echo of the Galactic Center Supernova Explosion that Produced Sgr A East
- Chemical abundances in Sgr A East: evidence for a Type Iax supernova remnant
- High-Energy X-rays from J174545.5-285829, the Cannonball: A Candidate Pulsar Wind Nebula Associated with Sgr A East
- XMM-Newton observations of the Galactic Centre Region - II: The soft thermal emission
- X-ray spectra of Sgr A East and diffuse X-ray background near the Galactic center
- The X-ray footprint of the CircumNuclear Disk
- Heating the intergalactic medium by radiative decay of neutrinos
- Atomic Carbon in the Central Molecular Zone of the Milky Way : Possible Cosmic-ray Induced Chemistry or Time-Dependent Chemistry Associated with SNR Sagittarius A East
- Observational evidences for the existence of 17.4 keV decaying degenerate sterile neutrinos near the Galactic Center
- Hydrodynamic Evolution of Sgr A East: The Imprint of A Supernova Remnant in the Galactic Center
- The contribution of young core-collapse supernova remnants to the X-ray emission near quiescent supermassive black holes
- Decaying Sterile Neutrinos as a Heating Source in the Milky Way Center
- Can decaying sterile neutrinos account for all dark matter?
- Indirect evidence of GeV Dark Matter
- High Energy Activity of the Super-Massive Black Hole at the Galactic Center
- High Energy Emission from the Galactic Center