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Fr.: densité de vecteur
meydân-e bordâri (#)
Fr.: champ vectoriel
Fr.: fonction vectorielle
A function whose value at each point is n-dimensional, as compared to a scalar function, whose value is one-dimensional.
Fr.: meson vectoriel
Any particle of unit spin, such as the W boson, the photon, or the rho meson.
Fr.: perturbation vectorielle
Fr.: produit vectoriel
Of two vectors, a vector whose direction is perpendicular to the plane containing the two initial vectors and whose magnitude is the product of the magnitudes of these vectors and the sine of the angle between them: A x B = C, C = |AB sin α|. The direction of C is given by the → right-hand screw rule. Same as → cross product. See also → scalar product.
fazâ-ye bordâri (#)
Fr.: espace vectoriel
A system of mathematical objects consisting of a set of (muultidimensional) vectors associated with a set of (one-dimensional) scalars, such that vectors can be added together and vectors can be multiplied by scalars while preserving the ordinary arithmetic properties (associativity, commutativity, distributivity, and so forth).
Vega (α Lyr)
Vâqe', Nasr-e Vaqe' (#)
The brightest star in the constellation → Lyra and the 5th brightest star in the sky. It is an A type → main sequence star of visual magnitude 0.03. Vega is also one of the closer stars to the Earth, lying just 25.0 light-years away. Vega's axis of rotation is nearly pointing at the Earth, therefore it is viewed pole-on. Fast rotation has flattened Vega at its poles, turning it from a sphere into an oblate spheroid. The polar diameter of Vega is 2.26 times that of the Sun, and its equatorial diameter 2.75 solar. The poles are therefore hotter (10,150 K) than the equator (7,950 K).
Vega, from Ar. al-Waqi' contraction of
an-Nasr al-Waqi' (
1) sabzijât; 2) giyâhi
1) Any of various herbaceous plants having parts that are used as food,
such as peas, beans, cabbage, potatoes, cauliflower, and onions.
Of, relating to, or characteristic of plants.
1) To grow or sprout as a plant by nutriment imbibed through roots and leaves.
Ultimately from L. vegetatus, p.p. of vegetare "to enliven, to animate," from vegetus "vigorous, enlivened, active," from vegere "to be alive, active;" akin to Skt. vaja- "force, strength;" PIE root *weg- "to be strong, be lively."
Giyâhidan, infinitive forum giyâh, → plant.
1) All the plants or plant life of a place.
Verbal noun from → vegetate.
1) Of, relating to, or characteristic of plants or their growth.
1) A piece of opaque or transparent cloth worn by women as a covering for the
head and shoulders.
M.E. veile; O.Fr. voile "a head-covering" (also "sail"), from L. vela, plural of velum "curtain, covering; sail."
Vâšâmé "veil," variants vâšâm, bâšâmé, bâšâm, from Mid.Pers. *varšâmak (loaned in Arm. varšamak "veil, scarf"); cf. Sogd. wâršâmé "veil;" from Proto-Ir. *varšāmaka-, from *varšām-, from *varš-, from var- "to cover;" cf. Av. var- "to cover, conceal;" Skt. var- "to cover;" Mid.Pers. warr "garment," prefixed uzvâr-, uzvârdan "to uncover, show, apprehend, interprete;" Mod.Pers. šalvâr "trousers" (literally "thigh cover;" the first component šal "thigh," šelang "thigh; step, distance between feet when walking," cognate with Gk. skelos "leg"); Kurd. (Soriani) barg "cover; clothes," da barg girtin "to wrap in a cover."
Fr.: Nébuleuse du Voile
1) General: An act of covering with or as if with a veil.
Verbal noun from veil (v.).
Any of the tubes forming part of the blood circulation system of the body, carrying mainly oxygen-depleted blood towards the heart (OxfordDictionaries.com).
M.E. veine, from O.Fr. veine "vein, artery, pulse," from L. vena "a blood vessel," also "a water course, a vein of metal," of unknown origin.
The Sail. A part of the constellation Argo in the Southern hemisphere, which was later divided into three parts, the others being Carina and Puppis. Vela is situated at about 10h right ascension, -50° declination. Abbreviation: Vel; Genitive: Velorum.
From L. vela, plural of velum "sail, curtain, covering," velare "to cover, veil."
pulsâr-e Bâdbân, tapâr-e ~
Fr.: pulsar du Voile
A pulsar with a short period (89 milliseconds) associated with the → Vela supernova remnant. It is approximately 1500 light-years distant. The Vela pulsar is one of the few pulsars detectable optically. Its optical flashes, of visual magnitude 26, were detected in 1977. Also named PSR 0833-45.
Vela supernova remnant
bâzmânde-ye abar-now-axtar-e Bâdbân
Fr.: reste de supernova du Voile
A → supernova remnant located in the southern Milky Way in the constellation → Vela. It has a large angular diameter of about 8° and lies 250 ± 30 pc away (Cha et al. 1999, ApJ 515, L25). Its overall emission is dominated by the interaction of the → supernova blast wave with the → interstellar medium. This SNR is also notable for a number of protrusions extending well beyond its rim, which were suggested to be fragments of ejecta from the supernova explosion. X-ray spectroscopy has since confirmed several of these protrusions to indeed be strongly enriched with ejecta. The age of the SNR is estimated to be ~11,000 years, based on the spin-down rate of the associated → Vela pulsar, but ages as large as 20,000-30,000 years have also been argued.