Detection of helium lines in Balmer-dominated shocks of Type Ia SNRs reveals enhanced helium in some remnants and challenges shock models, enabling new constraints on progenitor environments.
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3 Pith papers cite this work. Polarity classification is still indexing.
3
Pith papers citing it
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2026 3representative citing papers
Discovery of a narrow constant-width H-alpha trail in the Cygnus Loop, interpreted as a Balmer-dominated non-radiative shock from the SNR encountering dense material or magnetic structure edge-on.
UV background suppresses NEI in galaxy haloes, restoring equilibrium shock thresholds and producing extended absorption columns for OVI, CIV, and HI beyond the virial radius.
citing papers explorer
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Helium emission from Balmer-dominated shocks in Type Ia supernova remnants provides constraints to their progenitor systems
Detection of helium lines in Balmer-dominated shocks of Type Ia SNRs reveals enhanced helium in some remnants and challenges shock models, enabling new constraints on progenitor environments.
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Discovery of an extremely narrow trail-like feature crossing the Veil Supernova Remnant in deep amateur observations
Discovery of a narrow constant-width H-alpha trail in the Cygnus Loop, interpreted as a Balmer-dominated non-radiative shock from the SNR encountering dense material or magnetic structure edge-on.
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Non-Equilibrium Ionisation in Photoionised Haloes: Implications for Shock Stability and Absorption-Line Signatures
UV background suppresses NEI in galaxy haloes, restoring equilibrium shock thresholds and producing extended absorption columns for OVI, CIV, and HI beyond the virial radius.