Results 81 to 90 of about 62,408 (256)

OXIDATION‐DEFORMYLATION CASCADE CATALYZED BY A MONONUCLEAR COPPER COMPLEX

open access: yesChemistry – A European Journal, Accepted Article.
In this study, two copper complexes were synthesized using N3 (arising from two pyridines and one amide group) containing ligands N‐(2‐picolyl)picolinamide (L1H) and bis(2‐pyridylcarbonyl)amine (L2H), forming [(L1)CuII(OH2)(NO3)] (1) and [(L2)CuII(OH2)2](NO3) (2).
Yongxing Wang   +8 more
wiley   +1 more source

The physics of asymmetric supernovae and supernovae remnants [PDF]

open access: yesAdvances in Applied Physics, 2018
We model the circumstellar medium with four density profiles: hyperbolic type, power law type, exponential type and Gaussian type. We solve analytically or numerically the four first-order differential equations which arise in the framework of the classical thin layer approximation.
openaire   +4 more sources

Exploiting a New Strategy to Prepare Water‐Soluble Heteroleptic Iridium(III) Complexes to Control Electrochemiluminescence Reaction Pathways in Aqueous Solution

open access: yesChemistry – A European Journal, Accepted Article.
The direct derivatisation of heteroleptic iridium(III) complexes with sulfonate groups removes the limitations of prior strategies for the preparation of water‐soluble analogues, in which complexes were prepared from a narrow range of ligands with suitably polar or charged functional groups.
Kesha Sriee Manimaran   +7 more
wiley   +1 more source

Neutrino flavor instabilities in a time-dependent supernova model

open access: yesPhysics Letters B, 2015
A dense neutrino medium such as that inside a core-collapse supernova can experience collective flavor conversion or oscillations because of the neutral-current weak interaction among the neutrinos.
Sajad Abbar, Huaiyu Duan
doaj   +1 more source

Supernova Dust Evolution Probed by Deep-sea 60Fe Time History

open access: yesThe Astrophysical Journal, 2023
There is a wealth of data on live, undecayed ^60 Fe ( t _1/2 = 2.6 Myr) in deep-sea deposits, the lunar regolith, cosmic rays, and Antarctic snow, which is interpreted as originating from the recent explosions of at least two near-Earth supernovae.
Adrienne F. Ertel   +3 more
doaj   +1 more source

SOUSA's Swift Supernova Siblings [PDF]

open access: yesarXiv, 2015
Swift has observed over three hundred supernovae in its first ten years. Photometry from the Ultra-Violet Optical Telescope (UVOT) is being compiled in the Swift Optical/Ultraviolet Supernovae Archive (SOUSA). The diversity of supernovae leads to a wide dynamic range of intrinsic properties.
arxiv  

Circumstellar Nebulae in Young Supernova Remnants [PDF]

open access: yes, 2000
Supernovae descendent from massive stars explode in media that have been modified by their progenitors' mass loss and UV radiation. The supernova ejecta will first interact with the circumstellar material shed by the progenitors at late evolutionary stages, and then interact with the interstellar material.
arxiv   +1 more source

Modelling the progenitors of Core-Collapse Supernovae [PDF]

open access: yesarXiv, 2004
We present details of our investigation of the progenitors to core-collapse supernovae. We discuss observations and the theory of the lowest-mass stars to explode as supernovae.
arxiv  

SNO and supernovae [PDF]

open access: yesNuclear Physics B - Proceedings Supplements, 2001
The Sudbury Neutrino Observatory (SNO) has unique capabilities as a supernova detector. In the event of a galactic supernova there are opportunities, with the data that SNO would collect, to constrain certain intrinsic neutrino properties significantly, to test details of the various models of supernova dynamics, and to provide prompt notification to ...
openaire   +3 more sources

Combining Low‐Valent AlI and SnII Metal Centers for Small Molecule Activation

open access: yesEuropean Journal of Inorganic Chemistry, Accepted Article.
Reaction of the AlI complex (DIPPBDI‐H)AlˉK+ with the SnII complex (DIPPBDI)SnCl gave (DIPPBDI‐H)AlSn(DIPPBDI) (1); DIPPBDI = HC[C(Me)N(DIPP)]2, DIPP = 2,6‐diisopropylphenyl, DIPPBDI‐H = H2C=C(N‐DIPP)‐C(H)=C(Me)‐N‐DIPP. The crystal structure shows an asymmetric complex with a planar but strongly distorted trigonal coordination geometry at Al and ...
Tristan Löwl   +6 more
wiley   +1 more source

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