X- and Gamma-ray Studies of Cas A: Exposing Core Collapse to the Core
arXiv:astro-ph/0310518 · doi:10.1016/j.newar.2003.11.008
Abstract
In this review of X-ray and gamma-ray observations of Cas A, evidence is discussed that Cas A was a Type Ib supernova of a Wolf-Rayet star with a main sequence mass between 22-25 Msun, that exploded after stellar wind loss had reduced its mass to ~6 Msun. The observed kinematics and the high Ti-44 yield indicate that the supernova explosion was probably assymetric, with a kinetic energy of ~2x10^51 erg.
6 pages, 3 figures, to be published in New Astronomy Reviews (proceedings of the Workshop "Astronomy with Radioactivities IV and Filling the Sensitivity Gap in MeV Astronomy", Seeon, Germany, May 26-30, 2003)
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Cited by in corpus (31)
- Supernova remnants: the X-ray perspective
- A Million-Second Chandra View of Cassiopeia A
- Supernova remnant energetics and magnetars: no evidence in favour of millisecond proto-neutron stars
- Production and Distribution of Ti and Ni in a Three-dimensional Supernova Model Resembling Cassiopeia A
- The signature of 44Ti in Cassiopeia A revealed by IBIS/ISGRI on INTEGRAL
- Nuclear-Astrophysics Lessons from INTEGRAL
- Discovery of Outlying, High-Velocity Oxygen-Rich Ejecta in Cassiopeia A
- An HST Survey of the Highest-Velocity Ejecta in Cassiopeia A
- A JWST Survey of the Supernova Remnant Cassiopeia A
- The hydrodynamics of the supernova remnant Cas A: The influence of the progenitor evolution on the velocity structure and clumping
- The 40Ca(alpha,gamma)44Ti reaction in the energy regime of supernova nucleosynthesis
- Jets as diagnostics of the circumstellar medium and the explosion energetics of supernovae: the case of Cas A
- ejecta in young supernova remnants
- An INTEGRAL/IBIS view of Young Galactic SNRs through the 44Ti gamma-ray lines
- Supernova remnants with magnetars: clues to magnetar formation
- Element Abundances in the Unshocked Ejecta of Cassiopeia A
- Hard X-ray emissions from Cassiopeia A observed by INTEGRAL
- Gamma-ray Observations of Explosive Nucleosynthesis Products
- Molecular gas toward supernova remnant Cassiopeia A
- A Sub-Solar Metallicity Progenitor for Cassiopeia A, the remnant of a Type IIb Supernova
- High spatial resolution X-ray spectroscopy of SNR Cassiopeia A with {\sl Chandra}
- Is Supernova Remnant Cassiopeia A a PeVatron?
- Constraints on the kinematics of the 44Ti ejecta of Cassiopeia A from INTEGRAL/SPI
- X-ray diagnostics of Cassiopeia A's "Green Monster": evidence for dense shocked circumstellar plasma
- Discovery of Stable Titanium at the Northeastern Jet of Cassiopeia A: Need for a Weak Jet Mechanism?
- X-ray emitting structures in the Vela SNR: ejecta anisotropies and progenitor stellar wind residuals
- X-ray Studies of the Inverted Ejecta Layers in the Southeast Area of Cassiopeia A
- Near-Infrared Spectroscopy of Dense Ejecta Knots in the Outer Eastern Area of the Cassiopeia A Supernova Remnant
- New insights from cosmic gamma rays
- Gamma-ray line measurements from supernova explosions
- The forward and reverse shock dynamics of Cassiopeia A