Results 81 to 90 of about 63,717 (334)
Timing the starburst-AGN connection [PDF]
, 2010 The mass of super massive black holes at the centre of galaxies is tightly correlated with the mass of the galaxy bulges which host them. This observed correlation implies a mechanism of joint growth, but the precise physical processes responsible are a ...
Charlot, Stephane +2 more
core +2 more sources
Deciphering Small Molecule Diffusion Parameters Across Light Responsive Polymersome Membranes
Advanced Functional Materials, EarlyView.Light‐responsive polymersomes bearing donor–acceptor Stenhouse adducts (DASAs) enable programmable control over small‐molecule transport across synthetic membranes. By systematically varying DASA density, an optimal functionalization regime is identified that maximizes light‐gated permeability.
Farzina Matubbar +7 more
wiley +1 more source
Phenomenological Analogies in Black Hole Systems of all Masses
, 2004 I review the progress made on the physics of relativistic jets from black hole systems in the context of the analogy between AGN and microquasars that was proposed one decade ago.
Mirabel, I. F.
core +2 more sources
The Angular Momenta of Neutron Stars and Black Holes as a Window on Supernovae [PDF]
, 2011 It is now clear that a subset of supernovae display evidence for jets and are observed as gamma-ray bursts. The angular momentum distribution of massive stellar endpoints provides a rare means of constraining the nature of the central engine in core ...
Miller, J. M. +2 more
core +1 more source
2D Magnetic and Topological Quantum Materials and Devices for Ultralow Power Spintronics
Advanced Functional Materials, EarlyView.2D magnets and topological quantum materials enable ultralow‐power spintronics by combining robust magnetic order with symmetry‐protected, Berry‐curvature‐driven transport. Fundamentals of 2D anisotropy and spin‐orbit‐coupling induced band inversion are linked to scalable growth and vdW stacking.
Brahmdutta Dixit +5 more
wiley +1 more source
Confronting Models of Massive Star Evolution and Explosions with Remnant Mass Measurements
, 2017 The mass distribution of compact objects provides a fossil record that can be studied to uncover information on the late stages of massive star evolution, the supernova explosion mechanism, and the dense matter equation of state.
Raithel, Carolyn A. +2 more
core +1 more source
Binary black hole growth by gas accretion in stellar clusters [PDF]
, 2019 We show that binaries of stellar-mass black holes formed inside a young protoglobular cluster, can grow rapidly inside the cluster's core by accretion of the intracluster gas, before the gas may be depleted from the core.
Kazanas, Demosthenes, Roupas, Zacharias
core +3 more sources
Effect of mass-loss due to stellar winds on the formation of supermassive black hole seeds in dense nuclear star clusters [PDF]
, 2021 Arpan Das +3 more
openalex +1 more source
RETENTION OF STELLAR-MASS BLACK HOLES IN GLOBULAR CLUSTERS [PDF]
The Astrophysical Journal, 2013 Globular clusters should be born with significant numbers of stellar-mass black holes (BHs). It has been thought for two decades that very few of these BHs could be retained through the cluster lifetime. With masses ~10 MSun, BHs are ~20 times more massive than an average cluster star.
Morscher, Meagan +3 more
openaire +2 more sources
Advanced Functional Materials, EarlyView.ABSTRACT In this work, we introduce a trifluoromethoxy (OCF3) group as a pseudo‐halogen terminal group design for non‐fullerene acceptors, which combines strong inductive electron‐withdrawing ability with moderate resonance donation. The as‐synthesized BTP‐OCF3, when benchmarked against its methoxy analogue BTP‐OCH3, demonstrates narrowed bandgap ...
Chunliang Li +16 more
wiley +1 more source