Results 121 to 130 of about 13,120 (212)
86th Annual Meeting of the Meteoritical Society (2024)
Meteoritics &Planetary Science, Volume 59, Issue S1, Page A1-A468, August 2024.
wiley +1 more source
A Near-infrared Search for Helium in the Superluminous Supernova SN 2024ahr
We present a detailed study of SN 2024ahr, a hydrogen-poor superluminous supernova (SLSN-I), for which we determine a redshift of z = 0.0861. SN 2024ahr has a peak absolute magnitude of M _g ≈ M _r ≈ −21 mag, rest-frame rise and decline times (50% of ...
Harsh Kumar +15 more
doaj +1 more source
The binary-driven hypernova (BdHN) model has been introduced in the past years, to explain a subfamily of gamma-ray bursts (GRBs) with energies Eiso ≥ 1052 erg associated with type Ic supernovae.
Melon Fuksman J. D. +12 more
doaj +1 more source
The cosmic ray ionization and γ-ray budgets of star-forming galaxies. [PDF]
Krumholz MR, Crocker RM, Offner SSR.
europepmc +1 more source
A Detection of Helium in the Bright Superluminous Supernova SN 2024rmj
We present extensive ultraviolet, optical, and near-infrared (NIR) photometric and spectroscopic observations of the nearby hydrogen-poor superluminous supernova (SLSN-I) SN 2024rmj at z = 0.1189.
Harsh Kumar +10 more
doaj +1 more source
A nearby long gamma-ray burst from a merger of compact objects. [PDF]
Troja E +23 more
europepmc +1 more source
Supernova-induced Binary-interaction-powered Supernovae: A Model for SN2022jli
We present 3D hydrodynamical modelling of supernova (SN)-induced binary-interaction-powered SNe; a scenario proposed for the peculiar type Ic SN SN2022jli.
Ryosuke Hirai +6 more
doaj +1 more source
SN 2023syz and SN 2025cbj: Two Type IIn Supernovae Associated with IceCube High-energy Neutrinos
Type IIn supernovae (SNe IIn) are a subclass of core-collapse SNe in which strong interactions occur between the ejecta and dense circumstellar material, creating ideal conditions for the production of high-energy neutrinos.
Ming-Xuan Lu +3 more
doaj +1 more source
Detections of fast X-ray transients (FXTs) have accrued over the last few decades. However, their origin has remained mysterious. Rapid progress is now being made thanks to timely discoveries and localizations with the Einstein Probe mission.
Joyce N. D. van Dalen +32 more
doaj +1 more source
One of the open questions following the discovery of GW170817 is whether neutron star (NS) mergers are the only astrophysical sites capable of producing r -process elements.
Shreya Anand +43 more
doaj +1 more source

