activity
20122024
most citedA hot subdwarf-white dwarf super-Chandrasekhar candidate supernova Ia progenitor

66 citations · 548 across the 22 of their papers we have counts for

collaborators

22 papers

astro-ph.SR2024★ 5 cited

Evolution of binaries containing a hot subdwarf and a white dwarf to double white dwarfs, and double detonation supernovae with hypervelocity runaway stars

Abinaya Swaruba Rajamuthukumar, Evan B. Bauer, Stephen Justham +3

Compact binaries containing hot subdwarfs and white dwarfs have the potential to evolve into a variety of explosive transients. These systems could also explain hypervelocity runaw…

astro-ph.SR2024★ 11 cited

A spectroscopic and kinematic survey of fast hot subdwarfs

S. Geier, U. Heber, A. Irrgang +19

Hot subdwarfs (sdO/B) are the stripped helium cores of red giants formed by binary interactions. Close hot subdwarf binaries with massive white dwarf companions have been proposed…

astro-ph.HE2022★ 27 cited

SCATTER: A New Common Envelope Formalism

Rosanne Di Stefano, Matthias U. Kruckow, Yan Gao +2

One of the most mysterious astrophysical states is the common envelope (CE) phase of binary evolution, in which two stars are enshrouded by the envelope shed by one of them. Intera…

astro-ph.SR2022★ 21 cited

Triple evolution: an important channel in the formation of type Ia supernovae

Abinaya Swaruba Rajamuthukumar, Adrian Hamers, Patrick Neunteufel +2

Type Ia supernovae (SNe Ia) are thought to be the result of thermonuclear explosions in white dwarfs (WDs). Commonly considered formation pathways include two merging WDs (the doub…

astro-ph.SR2022★ 8 cited

The Equilibrium Tide: An Updated Prescription for Population Synthesis Codes

Holly P. Preece, Adrian S. Hamers, Patrick G. Neunteufel +2

We present an updated prescription for the equilibrium tides suitable for population synthesis codes. A grid of 1D evolutionary models was created and the viscous time-scale was ca…

astro-ph.SR2021★ 12 cited

Properties and applications of a predicted population of runaway He-sdO/B stars ejected from single degenerate He-donor SNe

P. Neunteufel, H. Preece, M. Kruckow +4

This study builds on previous works, producing the most extensive prediction of the properties of such a hypothetical population to date, taking into account both Chandrasekhar and…

astro-ph.SR2021★ 32 cited

A statistical view on stable and unstable Roche lobe overflow of a tertiary star onto the inner binary in triple systems

Adrian S. Hamers, Hila Glanz, Patrick Neunteufel

In compact stellar triple systems, an evolved tertiary star can overflow its Roche lobe around the inner binary. Subsequently, the tertiary star can transfer mass to the inner bina…

astro-ph.SR2021★ 66 cited

A hot subdwarf-white dwarf super-Chandrasekhar candidate supernova Ia progenitor

Ingrid Pelisoli, P. Neunteufel, S. Geier +8

Supernova Ia are bright explosive events that can be used to estimate cosmological distances, allowing us to study the expansion of the Universe. They are understood to result from…

astro-ph.SR2021★ 54 cited

A Catalogue of Potential Post Common Envelope Binaries

Matthias U. Kruckow, Patrick G. Neunteufel, Rosanne Di Stefano +2

We present a catalogue containing 839 candidate post common envelope systems. Common envelope evolution is very important in stellar astrophysics, particularly in the context of ve…

astro-ph.SR2021★ 33 cited

Return of the TEDI: revisiting the Triple Evolution Dynamical Instability channel in triple stars

Adrian S. Hamers, Hagai B. Perets, Todd A. Thompson +1

Triple-star systems exhibit a phenomenon known as the Triple Evolution Dynamical Instability (TEDI), in which mass loss in evolving triples triggers short-term dynamical instabilit…

astro-ph.HE2021★ 31 cited

First and second-generation black hole and neutron star mergers in 2+2 quadruples: population statistics

Adrian S. Hamers, Giacomo Fragione, Patrick Neunteufel +1

Recent detections of gravitational waves from mergers of neutron stars (NSs) and black holes (BHs) in the low and high-end mass gap regimes pose a puzzle to standard stellar and bi…

astro-ph.SR2020★ 13 cited

Predicted spatial and velocity distributions of ejected companion stars of helium accretion-induced thermonuclear supernovae

P. Neunteufel, M. Kruckow, S. Geier +1

Thermonuclear supernovae (SNe), a subset of which are the highly important SNe Type\,Ia, remain one of the more poorly understood phenomena known to modern astrophysics. In recent…

astro-ph.SR2020★ 60 cited

Multiple Stellar Evolution: a population synthesis algorithm to model the stellar, binary, and dynamical evolution of multiple-star systems

Adrian S. Hamers, Antti Rantala, Patrick Neunteufel +2

In recent years, observations have shown that multiple-star systems such as hierarchical triple and quadruple-star systems are common, especially among massive stars. They are pote…

astro-ph.SR2020★ 25 cited

Velocity limits in the thermonuclear supernova ejection scenario for hypervelocity stars and the origin of US 708

Patrick Neunteufel

Hypervelocity stars (HVS) are a class of stars moving at high enough velocities to be gravitationally unbound from the Galaxy. Ejection from a close binary system in which one of t…

astro-ph.EP2020★ 18 cited

TW Hya: an old protoplanetary disc revived by its planet

Sergei Nayakshin, Takashi Tsukagoshi, Cassandra Hall +6

Dark rings with bright rims are the indirect signposts of planets embedded in protoplanetary discs. In a recent first, an azimuthally elongated AU-scale blob, possibly a planet, wa…

astro-ph.SR2019★ 25 cited

The Evolution of Helium Star Plus Carbon-Oxygen White Dwarf Binary Systems and Implications for Diverse Stellar Transients and Hypervelocity Stars

P. Neunteufel, S. -C. Yoon, N. Langer

Helium accretion induced explosions in CO white dwarfs (WDs) are considered promising candidates for a number of observed types of stellar transients, including supernovae (SNe) of…

astro-ph.SR2016★ 36 cited

Models for the evolution of close binaries with He-Star and WD components towards Type Ia supernova explosions

P. Neunteufel, S. -C. Yoon, N. Langer

Type Ia supernovae (SNe Ia) have been an important tool for astronomy for quite some time; however, the nature of their progenitors remains somewhat mysterious. Recent theoretical…

astro-ph.IM2014★ 14 cited

Feasibility of radar detection of extensive air showers

J. Stasielak, R. Engel, S. Baur +4

Reflection of radio waves off the short-lived plasma produced by the high-energy shower particles in the air is simulated, considering various radar setups and shower geometries. W…

astro-ph.IM2014★ 45 cited

First Experimental Characterization of Microwave Emission from Cosmic Ray Air Showers

R. Smida, F. Werner, R. Engel +55

We report the first direct measurement of the overall characteristics of microwave radio emission from extensive air showers. Using a trigger provided by the KASCADE-Grande air sho…

astro-ph.HE2013★ 1 cited

Enhancement of the radar signal of air showers due to time compression

J. Stasielak, S. Baur, R. Engel +5

We investigate the feasibility of detecting extensive air showers by the radar technique at viewing angles smaller than to the shower axis. Considering a bistatic r…

astro-ph.IM2013★ 4 cited

Observation of Polarised Microwave Emission from Cosmic Ray Air Showers

R. Smida, F. Werner, R. Engel +55

We report on the first direct measurement of the basic features of microwave radio emission from extensive air showers. Using a trigger provided by the KASCADE-Grande air shower ar…

astro-ph.HE2012★ 7 cited

Radar reflection off extensive air showers

J. Stasielak, S. Baur, M. Bertaina +24

We investigate the possibility of detecting extensive air showers by the radar technique. Considering a bistatic radar system and different shower geometries, we simulate reflectio…