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double white dwarf sefid kutule-ye dotâyi Fr.: naine blanche double A → double-lined binary with two → white dwarf components. Short-period double white dwarfs can lose → orbital angular momentum by emitting → gravitational radiation and if the total mass of the binary exceeds the → Chandrasekhar limit, their eventual → merger might produce a → Type Ia supernova. |
double-degenerate binary system râžmân-e dorin-e dobâr vâgen Fr.: système binaire doublement dégénéré A system of evolved → binary stars in which both → components have ejected their envelopes and evolve toward → white dwarf stage. So far a half dozen double-degenerate → binary systems are known, for example Henize 2-248 (M. Santander-Garcia et al., 2015, 518, 5). → double; → degenerate; → binary; → system. |
double-diffusive convection hambaz-e do paxši Fr.: An instability involving two layers of fluid with opposite gradients of properties. Same as → fingering instability. See also → salt finger. Double-diffusive instabilities commonly occur in any astrophysical fluid that is stable according to the → Ledoux criterion, as long as the entropy and chemical stratifications have opposing contributions to the dynamical stability of the system. They drive weak forms of convection, and can cause substantial heat and compositional → mixing. Two cases can be distinguished. In fingering convection, entropy is stably stratified (∇ - ∇ad < 0), but chemical composition is unstably stratified (∇μ < 0); it is often referred to as → thermohaline convection by analogy with the oceanographic context in which the instability was first discovered. In oscillatory double-diffusive convection, entropy is unstably stratified (∇ - ∇ad > 0), but chemical composition is stably stratified (∇μ > 0); it is related to semiconvection, but can occur even when the → opacity is independent of composition (P. Garaud, 2014, arXiv:1401.0928). |
double-lined binary dorin-e doxatté Fr.: binaire à double raies A → spectroscopic binary in which the → spectral lines of both stars are seen and the lines are alternatively double and single. Same as → SB2 binary. See also: → single-lined binary. |
double-lined eclipsing binary dorin-e gerefti-ye doxatté Fr.: binaire à éclipse à double raies A → double-lined spectroscopic binary whose → light curve is typical of an → eclipsing binary. |
double-lined spectroscopic binary dorin-e doxatte-ye binâbnemâyik Fr.: binaire spectroscopique à double raies Same as → double-lined binary. → double; → line; → spectroscopic; → binary. |
double-lobed radio source xan-e râdioyi bâ lap-e dotâyi Fr.: radio source à double lobe A → galaxy that emits radio energy from two regions located on opposite sides of the galaxy. |
double-slit experiment âzmâyeš-e šekâf-e dotâyi (#) Fr.: expérience de double fente An experiment of → diffraction and → interference of two light beams using a → double slit; → Young's experiment. → double; → slit; → experiment. |
doublet dotâyé Fr.: doublet A pair of forbidden spectral lines of the same atom arising from
a common upper excitation level, for example [O III] λ 5007 and
[O III] λ 4959, [N II] λ 6584 and [N II] λ 6548, and [S II] λ 6717,
[S II] λ 6731. From O.Fr. doublet, from → double + -et diminutive suffix. Dotâyé, from dotâ→ double + -(y)é nuance suffix. |
doubly dobâr-, dv-, dotâyi Fr.: double, à ~ 1) To a double measure or degree. |
doubly convex do-kuž Fr.: double-convexe |
doubly ionized dobâr yonidé (#) Fr.: deux fois ionisé An atom that has lost two of its external electrons, for example O++ ([O III]). |
doubly refracting crystal bolur-e šakst-e dotâyi Fr.: cristal à double réfraction A → transparent → crystalline substance (such as calcite, quartz, and tourmaline) that is → anisotropic relative to the → speed of light. A ray incident normally on such crystals is broken up into two rays in traversing the crystal, → ordinary ray and → extraordinary ray. → doubly; → refracting; → crystal. |
doubt gomân (#), šakk (#), dodeli (#), Fr.: doute 1) A feeling of uncertainty about the truth, reality, or nature of something.
→ skepticism. M.E. douten, from O.Fr. douter "doubt, be doubtful," from L. dubitare "to doubt, question, hesitate" (related to dubius "uncertain"), from duo, "→ two," + habere "have, hold," with a sense of "of having two minds, undecided between two things;" cf. Pers. dodeli, as below. Gomân, from Mid.Pers. gumân "doubt;" ultimately from
Proto-Ir. *ui-man-, from suffixed *man- "to think,"
→ idea. |
down pâyin (#), foru Fr.: en bas, vers le bas Toward or in a lower physical position. M.E. doun, from O.E. dune "downward," short for adune, ofdune, from a-, of "off, from" + dune "hill." Pâyin "bottom, below; at the foot of," from
pâ(y) "foot; step;" Mid.Pers. pâd, pây; Av. pad- "foot;" cf.
Skt. pat; Gk. pos, genitive podos; L. pes,
genitive pedis; E. foot; Ger. Fuss; Fr. pied;
PIE *pod-/*ped-. |
downgrade forud-padâk, forud-padâkidan Fr.: déclasser, dévaloriser 1) A downward slope, especially of a road. |
download 1) bârgereftan; 2) bârgiri (#) Fr.: 1) télécharger; 2) téléchargement 1) To transfer data from any other computer to one's computer. Bârgereftan, literally "to take load," from bâr, → load, + gereftan "to take," → receiver; bârgiri, verbal noun of bârgereftan. |
downsizing bozorg-bé-kucak Fr.: A scenario of galaxy formation whereby massive galaxies formed earlier in the history of the → Universe (i.e. at high → redshifts) and completed their → star formation process more rapidly than low-mass galaxies. This scenario contrasts with what might be expected from simple → hierarchical structure formation scenarios, which predict that large galaxies formed in more recent times through the → merging of small galaxies. Downsizing, first suggested by Cowie et al. (1996, AJ 112, 839), from downsize (v.), is a new sense for this term. Its current main meaning in non astrophysical contexts is "to make in a smaller size, or become smaller in size (in particular in economic vocabulary, by reductions in personnel)," from → down + → size. Bozorg-bé-kucak, literally "large to small," from bozorg, → large, +bé "to" + kucak, → small. |
downstream forudâb (#) Fr.: en aval 1) With or in the direction of the current of a stream. → upstream. |
DQ white dwarf sefid kutule-ye DQ Fr.: naine blanche DQ A → white dwarf whose spectrum shows carbon features of any kind. |
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