The X-ray/radio and UV luminosity expected from symbiotic systems as the progenitor of SNe Ia

2016/01/31 by Xiangcun Meng, Zhanwen Han · 1 citation
Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysics and Cosmic Phenomena #Ejecta #Gamma-ray bursts and supernovae #Luminosity #Pair-instability supernova #Red giant #Supernova #White dwarf #astro-ph.HE #astro-ph.SR

paper · pdf · doi:10.1051/0004-6361/201526077

published as A&A 588, A88 (2016) · 12 pages, 5 figures, accepted for publication in A&A, after language editor

arxiv created 2016/02/09 · openalex publication_date 2016/02/09 · arxiv updated 2016/03/23 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Context. Symbiotic systems (i.e. a white dwarf + red giant star, WD + RG), which experience mass loss and form circumstellar material (CSM), have been suggested as being a possible progenitor system of type Ia supernovae (SNe Ia). After a supernova explosion, the supernova ejecta may interact with the CSM or the RG secondary. X-ray/radio emission (excess UV photons) is expected from the interaction between supernova ejecta and the CSM (RG secondary). However, no X-ray or radio emission that has originated from this type of system has been observationally detected, and only four SNe Ia have shown any possible signal of excess UV emission. These observational discrepancies need to be interpreted.

Citations

• Connecting RS Ophiuchi to [some] type Ia supernovae
• Measurements of Ω and Λ from 42 High‐Redshift Supernovae
• Recurrent Novae as a Progenitor System of Type Ia Supernovae. I. RS Ophiuchi Subclass: Systems with a Red Giant Companion
• The Delay-Time Distribution of Type Ia Supernovae and the Single-Degenerate Model
• A single-degenerate model for the progenitor of the Type Ia supernova 2002ic
• Accreting white dwarf models of Type I supernovae. III - Carbon deflagration supernovae
• X‐Ray, UV, and Optical Observations of Supernova 2006bp withSwift: Detection of Early X‐Ray Emission
• The fraction of type Ia supernovae exploding inside planetary nebulae (SNIPs)
• Presupernova evolution of accreting white dwarfs with rotation
• A SINGLE DEGENERATE PROGENITOR MODEL FOR TYPE Ia SUPERNOVAE HIGHLY EXCEEDING THE CHANDRASEKHAR MASS LIMIT
• Circumstellar Material in Type Ia Supernovae via Sodium Absorption Features
• On the evolution of rapidly rotating massive white dwarfs towards supernovae or collapses
• On the Hydrogen Emission from the Type Ia Supernova SN 2002ic
• Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
• TIDALLY ENHANCED STELLAR WIND: A WAY TO MAKE THE SYMBIOTIC CHANNEL TO TYPE Ia SUPERNOVA VIABLE
• Constraining the Type Ia Supernova Progenitor: The Search for Hydrogen in Nebular Spectra
• Binary population synthesis study of the supersoft X-ray phase of single degenerate type Ia supernova progenitors
• Companion Stars of Type Ia Supernovae
• The imprint of a symbiotic binary progenitor on the properties of Kepler’s supernova remnant
• SNe Ia as a cosmological probe
• Updated Opal Opacities
• Type Ia Supernova Explosion Models
• X-Ray Observations of Type Ia Supernovae with Swift : Evidence of Circumstellar Interaction for SN 2005ke

Cited by

• Blue Large-amplitude Pulsators: The Possible Surviving Companions of Type Ia Supernovae