Results 51 to 60 of about 8,271 (134)

Spatially resolved spectroscopy of faint star-forming galaxies & their environments in the high redshift universe [PDF]

open access: yes, 2011
This thesis is concerned with the spectroscopic observations of distant galaxies, 1 < z < 5. The galaxies presented here are intrinsically faint such that their ux is dominated by ordinary star formation rather than galaxy-galaxy merging and/or ...
Hurley, Mairéad
core  

Star polygons [PDF]

open access: yes, 2014
In mathematics we often encounter polygons, such us triangle, square, hexagon, etc., but we hardly encounter star polygons. Despite the fact that we do not meet them so often in mathematics, in nature they can be traced almost on every step.
Riosa, Blažka
core  

Star-Branched Polymers (Star Polymers)

open access: yes, 2015
The synthesis of well-defined regular and asymmetric mixed arm (hereinafter miktoarm) star-branched polymers by the living anionic polymerization is reviewed in this chapter.
Hadjichristidis, Nikos   +5 more
core   +1 more source

Dynamics and Equilibration Mechanisms in Block Copolymer Particles. [PDF]

open access: yesACS Polym Au, 2022
Lodge TP   +5 more
europepmc   +1 more source

Wavelength selective polymer network formation of end-functional star polymers

open access: yes, 2016
A wavelength selective technique for light-induced network formation based on two photo-active moieties, namely ortho-methylbenzaldehyde and tetrazole is introduced.
Kaupp, M.   +6 more
core   +1 more source

Physical properties of star-forming regions across the Galaxy

open access: yes, 2010
textThe Bolocam Galactic Plane Survey (BGPS) has surveyed the northern Galactic plane at 1.1 mm and detected 8,358 sources. The BGPS catalog is large enough to characterize the properties of massive star formation in a statistically significant way.
Dunham, Miranda Kay
core  

Star Centroiding Based on Fast Gaussian Fitting for Star Sensors

open access: yes, 2018
The most accurate star centroiding method for star sensors is the Gaussian fitting (GF) algorithm, because the intensity distribution of a star spot conforms to the Gaussian function, but the computational complexity of GF is too high for real-time ...
Guangjun Zhang   +4 more
core   +1 more source

Almost global existence for the Neumann problem of quasilinear wave equations outside star-shaped domains in 3D

open access: yes, 2017
In this article, we prove the almost global existence of solutions for quasilinear wave equations in the complement of star-shaped domains in three dimensions, with a Neumann boundary condition ...
Xin, Jie, Ren, Lulu
core   +1 more source

Strong almost finiteness [PDF]

open access: yes
A countable, bounded degree graph is almost finite if it has a tiling with isomorphic copies of finitely many F\o lner sets, and we call it strongly almost finite, if the tiling can be randomized so that the probability that a vertex is on the boundary ...
Timar, Adam, Elek, Gabor
core   +2 more sources

Structure and Asymptotic Theory for Nonlinear Models with GARCH Errors [PDF]

open access: yes
Nonlinear time series models, especially those with regime-switching and conditionally heteroskedastic errors, have become increasingly popular in the economics and finance literature.
Michael McAleer   +2 more
core  

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