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20232026
most citedSupernova Shocks Cannot Explain the Inflated State of Hypervelocity Runaways from White Dwarf Binaries

9 citations · 37 across the 18 of their papers we have counts for

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5 papers · 1 filter

astro-ph.HE2026

Cell-based theoretical criteria on the onset and stability limit of thermonuclear detonation

Kazuya Iwata, Keiichi Maeda, Ken J. Shen

One of the key unresolved problems in thermonuclear explosions of white dwarfs (WDs), including type Ia supernovae, is the condition for ignition and propagation of thermonuclear f…

astro-ph.HE2025★ 3 cited

Multiple outflows and delayed ejections revealed by early imaging of novae

Elias Aydi, John D. Monnier, Antoine Mérand +39

Novae are thermonuclear eruptions on accreting white dwarfs in interacting binaries. Although most of the accreted envelope is expelled, the mechanism -- impulsive ejection, multip…

astro-ph.HE2025★ 1 cited

Violent mergers revisited: The origin of the fastest stars in the Galaxy

Rüdiger Pakmor, Ken J. Shen, Aakash Bhat +12

Binary systems of two carbon-oxygen white dwarfs are one of the most promising candidates for the progenitor systems of Type Ia supernovae. Violent mergers, where the primary white…

astro-ph.HE2024★ 2 cited

Non-LTE Synthetic Observables of a Multidimensional Model of Type Ia Supernovae

Samuel J. Boos, Luc Dessart, Ken J. Shen +1

Many promising explosion models for the elusive origin of Type Ia supernovae (SNe Ia) ultimately fail to completely reproduce a number of observed properties of these events. One l…

astro-ph.HE2024★ 4 cited

Type Ia Supernovae Can Arise from the Detonations of Both Stars in a Double Degenerate Binary

Samuel J. Boos, Dean M. Townsley, Ken J. Shen

The precise origin of Type Ia supernovae (SNe Ia) is unknown despite their value to numerous areas in astronomy. While it is a long-standing consensus that they arise from an explo…