Results 91 to 100 of about 42,668 (331)

Relationship of Dye Adsorption Onto Biomass Activated Carbon Mixed Matrix Ultrafiltration: A Mass Transfer Model Study

open access: yesAdvanced Materials Interfaces, EarlyView.
This study explored dye molecule adsorption from water, focusing on activated carbon in polymer membranes for purifying low‐quality water. Polyvinylidene fluoride (PVDF) membranes showed enhanced removal efficiency of methylene blue (MB) from 89.29% to 98.33% with biomass‐activated carbon (BAC).
Khairul Anwar Mohamad Said   +5 more
wiley   +1 more source

Dynamics of Turbulent Convection and Convective Overshoot in a Moderate Mass Star

open access: yes, 2015
Continued progress in observational stellar astrophysics requires a deep understanding of the underlying convection dynamics. We present results of realistic 3D radiative hydrodynamic simulations of the outer layers of a moderate mass star (1.47 Msun ...
Kitiashvili, Irina N.   +3 more
core   +1 more source

The Evolution of Supermassive Population III Stars [PDF]

open access: yes, 2017
Supermassive primordial stars forming in atomically-cooled halos at $z \sim15-20$ are currently thought to be the progenitors of the earliest quasars in the Universe. In this picture, the star evolves under accretion rates of $0.1 - 1$ $M_\odot$ yr$^{-1}$
Haemmerlé, Lionel   +4 more
core   +2 more sources

Constraints on Magnetic Braking from the G8 Dwarf Stars 61 UMa and τ Cet

open access: yesThe Astrophysical Journal Letters, 2023
During the first half of their main-sequence lifetimes, stars rapidly lose angular momentum to their magnetized winds, a process known as magnetic braking.
Travis S. Metcalfe   +13 more
doaj   +1 more source

The treatment of mixing in core helium burning models -- II. Constraints from cluster star counts

open access: yes, 2015
The treatment of convective boundaries during core helium burning is a fundamental problem in stellar evolution calculations. In Paper~I we showed that new asteroseismic observations of these stars imply they have either very large convective cores or ...
Campbell, Simon W.   +3 more
core   +1 more source

Architecture of an All‐In‐One Microfluidic Platform for Accelerated Cancer Seeding, Enhanced Spheroid Formation, and Dynamic Drug Screening Trials

open access: yesAdvanced Materials Technologies, EarlyView.
An all‐in‐one microfluidic platform consists of two‐layered PDMS channels integrated with a hydrogel microwell array. This platform enables flow‐driven tumor cell capture, enhanced spheroid formation within the microwells, and advective drug testing. ABSTRACT Effective cancer drug screening requires platforms that replicate the physiological complexity
Omar M. Rahman   +2 more
wiley   +1 more source

Magnetic Field Evolution for Crystallization-driven Dynamos in C/O White Dwarfs

open access: yesThe Astrophysical Journal
We investigate the evolution of magnetic fields generated by the crystallization-driven dynamo in carbon–oxygen white dwarfs (WDs) with masses ≲1.05 M _⊙ .
Matias Castro-Tapia   +2 more
doaj   +1 more source

Stellar Evolution with Enriched Surface Convection Zones. I. General Effects of Planet Consumption [PDF]

open access: yesThe Astrophysical Journal, 2005
29 pages, 10 figures, accepted for publication by the Astrophysical Journal; one reference ...
Cody, Ann Marie, Sasselov, Dimitar
openaire   +2 more sources

Microfluidic Engineering of Chitosan‐Coated Nanoemulsions for Controlled Release and Stability in Space Pharmaceutics

open access: yesAdvanced Materials Technologies, EarlyView.
Microfluidic engineering enables the fabrication of chitosan‐coated, melatonin‐loaded nanoemulsions with controlled release and enhanced physicochemical stability for space pharmaceutics. Interfacial biopolymer coating modulates droplet behavior under accelerated thermal stress and simulated microgravity.
Modupe Adebowale   +3 more
wiley   +1 more source

Planetary Radii across Five Orders of Magnitude in Mass and Stellar Insolation: Application to Transits [PDF]

open access: yes, 2006
To aid in the physical interpretation of planetary radii constrained through observations of transiting planets, or eventually direct detections, we compute model radii of pure hydrogen-helium, water, rock, and iron planets, along with various mixtures ...
J. Fortney, M. Marley, J. Barnes
semanticscholar   +1 more source

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