Abstract Type Ia supernovae (SNe Ia) play a key role in the fields of astrophysics and
cosmology. It is widely accepted that SNe Ia arise from thermonuclear explosions of white …

A new era of lunar exploration has begun bringing immense opportunities for science as
well. It has been proposed to deploy a new generation of observatories on the lunar surface …

We report a spectroscopic search for hypervelocity white dwarfs (WDs) that are runaways
from Type Ia supernovae (SNe Ia) and related thermonuclear explosions. Candidates are …

The double detonation is a widely discussed mechanism to explain Type Ia supernovae
from explosions of sub-Chandrasekhar mass white dwarfs. In this scenario, a helium …

We present optical photometric and spectroscopic observations of the 02es-like type Ia
supernova (SN) 2022ywc. The transient occurred in the outskirts of an elliptical host galaxy …

We perform nonlocal thermodynamic equilibrium (NLTE) model atmosphere analyses of the
three hottest hypervelocity stars (space velocities between≈ 1500–2800 km s− 1) known to …

Star-forming galaxies like the Milky Way are surrounded by a hot gaseous halo at the virial
temperature–the so-called galactic corona–that plays a fundamental role in their evolution …

Abstract Type Ia supernovae (SNe Ia) are securely understood to come from the
thermonuclear explosion of a white dwarf as a result of binary interaction, but the nature of …

The radioisotope 44Ti is produced through α-rich freezeout and explosive helium burning in
type Ia supernovae (SNe Ia). In this paper, we discuss how the detection of 44Ti, either …

We implement general relativistic hydrodynamics in the moving-mesh code arepo. We also
couple a solver for the Einstein field equations employing the conformal flatness …