Results 21 to 30 of about 257,269 (299)

The alignment is in their stars: on the spin-alignment of stars in star clusters [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society: Letters, 2018
ABSTRACT We simulate star formation in two molecular clouds extracted from a larger disc-galaxy simulation with a spatial resolution of ∼0.1 pc, one exiting a spiral arm dominated by compression, and another in an inter-arm region more strongly affected by galactic shear.
Rey-Raposo, Ramon, Read, Justin I
openaire   +5 more sources

On stars and Steiner stars

open access: yesDiscrete Optimization, 2009
AbstractA Steiner star for a set P of n points in Rd connects an arbitrary point in Rd to all points of P, while a star connects one of the points in P to the remaining n−1 points of P. All connections are realized by straight line segments. Let the length of a graph be the total Euclidean length of its edges.
Csaba D. Tóth   +2 more
openaire   +2 more sources

Rainbow’s stars [PDF]

open access: yesThe European Physical Journal C, 2017
In recent years, a growing interest on the equilibrium of compact astrophysical objects like white dwarf and neutron stars has been manifested. In particular, various modifications due to Planck scale energy effects have been considered. In this paper we analyze the modification induced by Gravity's Rainbow on the equilibrium configurations described ...
Garattini, Remo, Mandanici, Gianluca
openaire   +4 more sources

Health literacy as a challenge for health education

open access: yesSHS Web of Conferences, 2018
Scientific literature demonstrates a well-established correlation between education and health literacy; education and health outcomes; health literacy and health outcomes. Health literacy has a mediating role between education and health.
Stars I.
doaj   +1 more source

On stars and Steiner stars. II [PDF]

open access: yesProceedings of the Twentieth Annual ACM-SIAM Symposium on Discrete Algorithms, 2009
A {\em Steiner star} for a set $P$ of $n$ points in $\RR^d$ connects an arbitrary center point to all points of $P$, while a {\em star} connects a point $p\in P$ to the remaining $n-1$ points of $P$. All connections are realized by straight line segments. Fekete and Meijer showed that the minimum star is at most $\sqrt{2}$ times longer than the minimum
Guangwu Xu   +2 more
openaire   +2 more sources

Star Product and Star Exponential [PDF]

open access: yes, 2012
Here we extend the star products by means of complex symmetric matrices. In this way we obtain a family of star products. Next we consider the star exponentials with respect to these star products, and finally we obtain several interesting identities.
Tomihisa, Toshio, Yoshioka, Akira
openaire   +4 more sources

Moduli stars [PDF]

open access: yesJournal of High Energy Physics, 2018
AbstractWe explore the possibility that (Bose-Einstein) condensation of scalar fields from string compactifications can lead to long-lived compact objects. Depending on the type of scalar fields we find different realisations of star-like and solitonic objects.
Krippendorf, Sven   +2 more
openaire   +5 more sources

Unsupervised discovery of human activities from long‐time videos

open access: yesIET Computer Vision, 2015
In this study, the authors propose a complete framework based on a hierarchical activity model to understand and recognise activities of daily living in unstructured scenes.
Salma Elloumi   +4 more
doaj   +1 more source

NEW VARIABLE STAR IN THE ORION CONSTELLATION

open access: yesOdessa Astronomical Publications, 2017
New variable star with α = 05° 57m22s, δ = +20°15.5' (1950) was discovered with elements JD Max=2436999.28 + 0.2343973 E, range 15.6- 16.2m (pg) and asymmetry M-m=0.26.
I. S. Brjukhanov, V. P. Goranskij
doaj   +1 more source

Origin of Star-to-Star Abundance Inhomogeneities in Star Clusters [PDF]

open access: yesProceedings of the International Astronomical Union, 2008
AbstractThe mass reinserted by young stars of an emerging massive compact cluster shows a bimodal hydrodynamic behaviour. In the inner part of the cluster, it is thermally unstable, while in its outer parts it forms an out-blowing wind. The chemical homogeneity/inhomogeneity of low/high mass clusters demonstrates the relevance of this solution to the ...
S. Silich   +3 more
openaire   +3 more sources

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