Results 81 to 90 of about 4,667,827 (292)
Advanced Materials, EarlyView.Molecular doping of conjugated polymers is fundamentally constrained by thermodynamic phase behavior. This Perspective reframes doping efficiency and stability in terms of miscibility limits, binodals, and solvus boundaries, highlighting the role of effective interaction parameters and charge transfer.
Somayeh Kashani +10 more
wiley +1 more source
The Unexplored Dusty Nova LMCN 2009-05a in the Large Magellanic Cloud
The Astronomical JournalWe present a detailed spectrophotometric study of nova LMCN 2009-05a, located in the Large Magellanic Cloud (LMC). Photometric observations reveal a dust dip in the optical light curve, classifying it as a D-class nova.
Mohit Singh Bisht +6 more
doaj +1 more source
Detection of Two-armed Spiral Shocks on the Accretion Disk of the Eclipsing Fast Nova V1494 Aquilae [PDF]
The Astrophysical Journal, 2004 7 pages, 3 figurs, to appear in ...
Hachisu, Izumi +2 more
openaire +2 more sources
Second Timescale Photometry of the Very Fast Nova V1674 Her with Palomar Gattini-IR
Research Notes of the AAS, 2021 Abstract We report second-timescale infrared photometry of the nova V1674 Her using Palomar Gattini-IR (PGIR). These observations constitute the first infrared and highest temporal resolution data (resolution of ≈0.84 s) of the nova reported to date.
Kylie Y. Hansen +17 more
openaire +3 more sources
Poly(Alkoxythiophene) Rod‐Coil Block Copolymers for Organic Electrochemical Transistors
Advanced Materials, EarlyView.We present the first synthesis of poly(3‐alkoxythiophene) rod‐coil block copolymers as a new architecture for OMIECs. Incorporating PEG and PLLA coils can enhance device performance beyond the homopolymer. The figure‐of‐merit depends uniquely on coil length.
Junfu Tian +23 more
wiley +1 more source
KDU journal of multidisciplinary studiesWe present a comprehensive analysis of ultraviolet (UV) spectra from the International Ultraviolet Explorer (IUE) of three classical novae: OS And (Nova Andromedae 1986), QU Vul (Nova Vulpeculae 1984 No. 2), and V1974 Cyg(Nova Cygni 1992).
Theekshana Piyadasa, N. Medagangoda
semanticscholar +1 more source
Broad absorption line symbiotic stars: highly ionized species in the fast outflow from MWC 560 [PDF]
, 2018 In symbiotic binaries, jets and disk winds may be integral to the physics of accretion onto white dwarfs from cool giants. The persistent outflow from symbiotic star MWC 560 (=V694 Mon) is known to manifest as low-ionization broad absorption lines (BALs),
A. Lucy, C. Knigge, J. Sokoloski
semanticscholar +1 more source
Rms–flux relation and fast optical variability simulations of the nova-like system MV Lyr [PDF]
Monthly Notices of the Royal Astronomical Society, 2015 The stochastic variability (flickering) of the nova-like system (subclass of cataclysmic variable) MV Lyr yields a complicated power density spectrum with four break frequencies. Scaringi et al. (2012) analysed high-cadence Kepler data of MV Lyr, taken almost continuously over 600 days, giving the unique opportunity to study multicomponent Power ...
Dobrotka, A. +2 more
openaire +2 more sources
Advanced Materials Interfaces, EarlyView.Ba‐doped SrTiO3 perovskites establish a direct correlation between photoelectrochemical activity and photocatalytic performance. Optimized Ba0.5Sr0.5TiO3 exhibits enhanced charge separation, photocurrent generation, and visible‐light‐driven dye degradation through defect‐induced oxygen vacancies and lattice distortion.
Sagar A. Nikam +6 more
wiley +1 more source
Resolving different sources of fast X-ray variability of the dwarf nova RU Peg in quiescence★ [PDF]
Monthly Notices of the Royal Astronomical Society, 2014 accepted for publication in MNRAS, 12 pages, 8 figures, 1 ...
Dobrotka, A. +2 more
openaire +2 more sources