Results 51 to 60 of about 2,475,925 (212)
Observational constraints on the progenitor of core-collapse supernovae [PDF]
It is well-known that some massive stars evolve to an end state which results in the collapse of the stellar core, as the hydrostatic pressure can no longer support gravity, leading to powerful explosions called supernovae (SNe).
ELIAS DE LA ROSA, NANCY DEL CARMEN
core +1 more source
Detecting the progenitors of core-collapse supernovae [PDF]
A novel project to directly detect the progenitor stars of nearby core-collapse supernovae in pre-discovery archive images is briefly described.
openaire +4 more sources
Magnetorotational Instability in Core-Collapse Supernovae [PDF]
Proceedings in Acta Physica Polonica B, Proceedings Supplement, Vol. 10, No.
Rembiasz, T. +5 more
openaire +3 more sources
Equation of State Effects in Core-Collapse Supernovae [PDF]
We investigate the impact of different properties of the nuclear equation of state in core-collapse supernovae, with a focus on the proto-neutron-star contraction and its impact on the shock evolution. To this end, we introduce a range of equations of state that vary the nucleon effective mass, incompressibility, symmetry energy, and nuclear saturation
Yasin, H. +3 more
openaire +4 more sources
Long gamma-ray bursts and core-collapse supernovae have differentenvironments [PDF]
When massive stars exhaust their fuel they collapse andoften produce the extraordinarily bright explosions known ascore-collapse supernovae. On occasion, this stellar collapse also powersan even more brilliant relativistic explosion known as a long ...
C. Conselice +124 more
core +1 more source
Nuclei in core-collapse supernovae engine
Herein, we review the nuclear equations of state (EOSs) %for core-collapse supernova simulations and the constituent nuclei of core-collapse supernovae (CCSNe) and their roles in CCSN simulations. Various nuclei such as deuterons, iron, and extremely neutron-rich nuclei compose in the central engines of CCSNe.
S. Furusawa, H. Nagakura
openaire +2 more sources
Essential ingredients in core-collapse supernovae
Carrying 1044 joules of kinetic energy and a rich mix of newly synthesized atomic nuclei, core-collapse supernovae are the preeminent foundries of the nuclear species which make up our solar system and ourselves.
W. Raphael Hix +9 more
doaj +1 more source
The Progenitor of the S147 Supernova Remnant
The supernova remnant (SNR) S147 contains the pulsar PSR J0538+2817 and a likely unbound binary companion, HD 37424. It is the only good Galactic candidate for a binary unbound by a core-collapse supernova.
Elvira Cruz-Cruz +1 more
doaj +1 more source
Proprioception controls trunk straightness in trees through opposite tension wood formation. A spherical growth chamber (a), combined with a two‐dimensional rotating clinostat (b2), suppresses gravi‐ and phototropic sensing. The tree is first tilted horizontally (b1), triggering upward gravitropic bending, actuated by tension wood formation on the ...
Alexandre Caulus +7 more
wiley +1 more source
Presolar graphite grains carry the isotopic signatures of their parent stars. A significant fraction of presolar graphites show isotopic abundance anomalies relative to solar for elements such as O, Si, Mg, and Ca, which are compatible with ...
Marco Pignatari +10 more
doaj +1 more source

