Results 91 to 100 of about 151,210 (305)
Models of Accretion Disks [PDF]
An accretion flow onto a supermassive black hole is the primary process powering quasars. However, a geometry of this flow is not well constrained. Both global MHD simulations and observations suggest that there are several emission components present in the nucleus: an accretion disk, hot plasma (corona or sphere) with electrons scattering the optical
openaire +2 more sources
Genetically Programmed Shape‐Morphing of Engineered Living Materials
Here, bacterial and mammalian engineered living materials (ELMs) are presented, in which living cells direct genetically programmed and enzymatically mediated shape‐morphing. The resulting deformation and shape‐recovery can be actuated in a genetically controlled manner by an ELM incorporating out‐of‐equilibrium counteracting biochemical reactions with
Jan Becker +7 more
wiley +1 more source
WIND-DRIVEN ACCRETION IN TRANSITIONAL PROTOSTELLAR DISKS
Transitional protostellar disks have inner cavities that are heavily depleted in dust and gas, yet most of them show signs of ongoing accretion, often at rates comparable to full disks.
Goodman, Jeremy J., Wang, Lile
core +1 more source
Bioinspired Hydrogels with Broadly Programmable Mechanics for Soft‐Tissue Interfaces
Sea cucumber‐inspired gelatin hydrogels are formed by directional freezing and mechanically programmed through subsequent ionic treatment. Multiscale characterization and modeling link ion‐regulated chain interactions to directional load transfer within the aligned hierarchical architecture.
Youchao Teng +20 more
wiley +1 more source
The Effects of Complex Accretion Disk Geometry on Broadened Iron Ka Lines
X-rays are emitted from the corona above the orbiting matter of the accretion disk and either travel directly to the observer or illuminate the disk. Illumination of the inner disk is enhanced by gravitational light bending, which focuses the rays toward
William Surgent, Daniel R. Wilkins
doaj +1 more source
In a recent paper, Abramowicz, Czerny, Lasota and Szuszkiewicz (1988) have found a new branch of equilibrium solutions for stationary accretion discs around black holes. These solutions correspond to moderately super-Eddington accretion rates. The existence of the new branch is a consequence of cooling due to general relativistic Roche lobe overflow ...
M. A. Abramowicz +3 more
openaire +1 more source
Accretion disks around young stars: the cradles of planet formation
Protoplanetary disks around young stars are the birth sites of planetary systems like our own. Disks represent the gaseous dusty matter left after the formation of their central stars.
Richard D. Teague, Dmitry A. Semenov
core +1 more source
A degradable, skin‐conformal bioelectronic patch combines a starch‐dominated nanocomposite conductor with a gelatin substrate to enable sensitive strain sensing, high‐fidelity electrocardiography, electromyography, electrooculography, and machine‐learning‐assisted gesture control.
Ming Dong +10 more
wiley +1 more source
Eccentric Binaries Accreting from Thin Disks: Orbital Evolution
Circumbinary disks crucially affect the orbital and electromagnetic properties of binary systems across the Universe, from stars in our Galactic neighborhood to supermassive black hole binaries formed as the result of tumultuous galactic mergers ...
Alexander J. Dittmann +2 more
doaj +1 more source
Versatile guanosine‐quadruplex (GQ) hydrogels are developed as dynamic biomatrices for cell culture. These scaffolds are fabricated under mild aqueous conditions, present improved stability, tunable mechanical properties within physiological ranges; fibrillar, porous microstructure, ion conductivity, and cytocompatibility.
Neha Thakur +10 more
wiley +1 more source

