Type Ia Supernova Explosions in Binary Systems: A Review

ZW Liu, FK Röpke, Z Han - Research in Astronomy and …, 2023 - iopscience.iop.org
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 …

Observational properties of thermonuclear supernovae

SW Jha, K Maguire, M Sullivan - Nature Astronomy, 2019 - nature.com
The explosive death of a star as a supernova is one of the most dramatic events in the
Universe. Supernovae have an outsized impact on many areas of astrophysics: they are …

A kilonova as the electromagnetic counterpart to a gravitational-wave source

SJ Smartt, TW Chen, A Jerkstrand, M Coughlin… - Nature, 2017 - nature.com
Gravitational waves were discovered with the detection of binary black-hole mergers and
they should also be detectable from lower-mass neutron-star mergers. These are predicted …

The zwicky transient facility: science objectives

MJ Graham, SR Kulkarni, EC Bellm… - Publications of the …, 2019 - iopscience.iop.org
Abstract The Zwicky Transient Facility (ZTF), a public–private enterprise, is a new time-
domain survey employing a dedicated camera on the Palomar 48-inch Schmidt telescope …

Optical emission from a kilonova following a gravitational-wave-detected neutron-star merger

I Arcavi, G Hosseinzadeh, DA Howell, C McCully… - Nature, 2017 - nature.com
The merger of two neutron stars has been predicted to produce an optical–infrared transient
(lasting a few days) known as a 'kilonova', powered by the radioactive decay of neutron-rich …

An embedded X-ray source shines through the aspherical AT 2018cow: revealing the inner workings of the most luminous fast-evolving optical transients

R Margutti, BD Metzger, R Chornock… - The Astrophysical …, 2019 - iopscience.iop.org
We present the first extensive radio to γ-ray observations of a fast-rising blue optical
transient, AT 2018cow, over its first∼ 100 days. AT 2018cow rose over a few days to a peak …

Ultra-stripped supernovae: progenitors and fate

TM Tauris, N Langer… - Monthly Notices of the …, 2015 - academic.oup.com
The explosion of ultra-stripped stars in close binaries can lead to ejecta masses< 0.1 M⊙
and may explain some of the recent discoveries of weak and fast optical transients. In Tauris …

Opacities and spectra of the r-process ejecta from neutron star mergers

D Kasen, NR Badnell, J Barnes - The Astrophysical Journal, 2013 - iopscience.iop.org
Material ejected during (or immediately following) the merger of two neutron stars may
assemble into heavy elements through the r-process. The subsequent radioactive decay of …

A lanthanide-rich kilonova in the aftermath of a long gamma-ray burst

YH Yang, E Troja, B O'Connor, CL Fryer, M Im… - Nature, 2024 - nature.com
Observationally, kilonovae are astrophysical transients powered by the radioactive decay of
nuclei heavier than iron, thought to be synthesized in the merger of two compact objects …

PESSTO: survey description and products from the first data release by the Public ESO Spectroscopic Survey of Transient Objects

SJ Smartt, S Valenti, M Fraser, C Inserra… - Astronomy & …, 2015 - aanda.org
Context. The Public European Southern Observatory Spectroscopic Survey of Transient
Objects (PESSTO) began as a public spectroscopic survey in April 2012. PESSTO classifies …