Results 11 to 20 of about 168,490,903 (279)

Minimum drift times infer trajectories of ghost nets found in the Maldives [PDF]

open access: yes, 2020
This study explores methods to estimate minimum drift times of ghost nets found in the Maldives with the aim of identifying a putative origin. We highlight that percentage cover of biofouling organisms and capitulum length of Lepas anatifera are two ...
Souch, G.   +8 more
core   +1 more source

HARDNESS AND FRICTIONAL BEHAVIOUR OF DENTAL HYBRID COMPOSITE RESIN FILLED BY SILICON CARBIDE NANOFIBERS [PDF]

open access: yesJournal of the Egyptian Society of Tribology, 2022
The objectives of the present investigation is to determine the effect of light curing time on the hardness and friction coefficient of composite resin filled with (SiC NFs). The materials used are hybrid composite resin and SiC NFs.
A. K. Ameer   +3 more
doaj   +1 more source

The minimum water curing recovery time after burning of aluminium fiber light weight concrete (with alwa as coarse aggregate) modulus elasticity [PDF]

open access: yesAIP Conference Proceedings, 2019
The research concerns on the strength of light weight concrete with aluminum fiber as micro-reinforcement by environmental load especially burning and water curing. The purpose of this study was to determine the minimum time of water curing required to obtain full recovery of modulus elasticity.
Antonius Mediyanto   +3 more
openaire   +1 more source

Clumpy dust clouds and extended atmosphere of the AGB star W Hydrae revealed with VLT/SPHERE-ZIMPOL and VLTI/AMBER [PDF]

open access: yesAstronomy & Astrophysics, 2016
14 pages, 9 figures, accepted for publication in Astronomy and ...
Ohnaka, K., Weigelt, G., Hofmann, K.
openaire   +3 more sources

REDISCUSSION OF PER100 CHANGE OF THE CLOSE BINARY V65l CASSIOPEIAE [PDF]

open access: yesJournal of Astronomy and Space Sciences, 2002
Observations of times of minimum lights of the eclipsing binary V65l Cas were carried out on the three nights from November 21-23, 2000. From our observations a total of seven new times of minimum lights was obtained.
Chun-Hwey Kim   +4 more
doaj   +1 more source

A Photometric Study of Near-Contact Binary ZZ Aur [PDF]

open access: yesJournal of Astronomy and Space Sciences, 2002
The BVR CCD full light curves of ZZ Aur were obtained as one of the near-contact binary observing programs at the Sobaek Mt. Observatory during Feb. 2000 - Feb. 2001. From the present observations, three primary and seven secondary times of minimum light
Kyu-Dong Oh   +3 more
doaj   +1 more source

Surface plasmon polariton modification in top-emitting organic light-emitting diodes for enhanced light outcoupling [PDF]

open access: yes, 2014
We report on the enhanced light outcoupling efficiency of monochrome top-emitting organic light-emitting diodes (OLEDs). These OLEDs incorporate a hole transport layer (HTL) material with a substantially lower refractive index (∼ 1:5) than the emitter ...
Hofmann, S.   +13 more
core   +1 more source

Apsidal Motion Study of Close Binary System CW Cephei [PDF]

open access: yesJournal of Astronomy and Space Sciences, 2015
New observations for the times of minimum lights of a well-known apsidal motion star CW Cephei were made using a 0.6 m wide field telescope at Jincheon station of Chungbuk National University Observatory, Korea during the 2015 observational season.
Wonyong Han   +5 more
doaj   +1 more source

WASP light curve of the eclipsing binary VZ CVn [PDF]

open access: yesSerbian Astronomical Journal, 2012
The WASP light curve of the eclipsing binary VZ CVn, consisting of more than 14000 individual observations, is analyzed for photometric elements using the modeling code of Đurašević (1992).
Latković O.
doaj   +1 more source

The BV Photometry of the RR Lyrae Star, BH Ursae Majoris: Light Curves and Period Study [PDF]

open access: yesJournal of Astronomy and Space Sciences, 2011
The first presented BV light curves of BH UMa confirmed Krajci’s (2005) result that BH UMa is an RR Lyr star that belongs to the RRc subgroup. The light curves showed a slight asymmetry of D = 0.453 with an amplitude of about 0.m58 in B, 0.m47 in V ...
Chun-Hwey Kim, Jang Hae Jeong
doaj   +1 more source

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