Results 101 to 110 of about 6,421 (225)
Three-dimensional Structure of Incomplete Carbon–Oxygen Detonations in Type Ia Supernovae
Carbon–oxygen (CO) detonation with reactions terminating either after burning of ^12 C in the leading ^12 C + ^12 C reaction or after burning of ^12 C and ^16 O to Si-group elements may occur in the low-density outer layers of exploding white dwarfs and
A. Khokhlov +8 more
doaj +1 more source
Photometric typing of normal and peculiar type Ia supernovae
Indexación: ScopusWe present a new photometric typing technique for normal type Ia supernovae (SNe Ia) and peculiar SNe Ia such as SN 1991bg-like, type Iax and super-Chandrasekhar SNe Ia.
González-Gaitán, Santiago +1 more
core +1 more source
SN 2024gy: Multiepoch Spectroscopic Features Suggestive of Delayed Detonation in a Type Ia Supernova
We present photometric and spectroscopic observations of SN 2024gy, a Type Ia supernova (SN Ia) exhibiting high-velocity features (HVFs) in its early-time spectra. This SN reaches a peak B -band magnitude of −19.25 ± 0.29 mag and subsequently declines by
Liping Li +30 more
doaj +1 more source
Detection of Persistent Helium Absorption in the 91bg-like Type Ia Supernova 2022an
We present optical and near-infrared (NIR) observations of the fast-declining Type Ia supernova (SN Ia) 2022an. The photometric and spectroscopic properties identify it as a standard 91bg-like event; however, our data reveal a relatively narrow ...
Ping Chen +16 more
doaj +1 more source
Supernovae are some of the brightest and most energetic explosions in the universe. In the mid- to late-twentieth century, it was discovered that Type Ia supernovae, the brightest and most homogeneous subtype, are a different breed from the rest ...
Johnson, Traci Lin
core
SN 2023ehl: A Normal Type Ia Supernova with High-velocity Features
SN 2023ehl, a normal Type Ia supernova with a typical decline rate, was discovered in the galaxy UGC 11555 and offers valuable insights into the explosion mechanisms of white dwarfs.
Xiangyun Zeng +30 more
doaj +1 more source
Type Ia Supernovae Inside Planetary Nebulae (SNIPs)
We estimate that the fraction of type Ia supernovae (SNe Ia) exploding inside planetary nebulae (PNe), termed SNIPs, is at least 20%. We based this on (i) sodium absorption lines in some SN Ia, (ii) hydrogen emission line from circumstellar matter, and ...
D. Tsebrenko, N. Soker
core +1 more source
Turbulence-Flame Interaction on the Early Evolution of Flames in Type Ia Supernovae
Type Ia supernovae are bright stellar explosions thought to occur when a runaway thermonuclear reaction incinerates a compact star known as white dwarf (WD).
Jackson, Aaron P. +5 more
core
K-corrections and Extinction Corrections for Type Ia Supernovae [PDF]
The measurement of the cosmological parameters from Type Ia supernovae hinges on our ability to compare nearby and distant supernovae accurately. Here we present an advance on a method for performing generalized K-corrections for Type Ia supernovae which
Peter Nugent +5 more
core
The Hubble Constant from Blue Type Ia Supernovae
There is a persistent tension of about 5 σ –6 σ between the value of the Hubble constant, as derived from the local distance ladder versus the cosmic microwave background, signaling either unaccounted for systematics in the measurements or “new physics,”
Christa Gall +3 more
doaj +1 more source

