<< < "no abe acc act aff ama ani ant aps ast atm aut bar bic Boh bou cal car cel che cla col com com Com con con con con con con con con con con con con Cor cor cot cul de- dec dem des dif dil dir dis dom dyn Edd ele ele emi equ Eve exc exp fac fin for fre fuz gen Glo gra gra Ham hel hor hyd ign inc inf Inf int Int int ion irr jum Lag lea lig lin Lor Lyo mag mat met min Mon moo NaC neg New New non non non nul obs one opt Ori oxi par per per phl pho pla Pla pol pos pre pro pro pse qua rad rad rea rec reg rel res ret rot Ryd sci sec sec seq sim Sod sor spe sta ste sto sub sup syn the Tho Tor tra tru und vec vio wav Wil zir > >>
comparison star setâre-ye hamsanješ Fr.: étoile de comparaison A non-variable star used to monitor the variations of another nearby star. → comparison; → star. |
competition hâjuyeš Fr.: compétition 1) The act of competing; rivalry for supremacy, a prize, etc. 2) A contest for some prize, honor, or advantage (Dictionary.com). |
competitive accretion model model-e farbâl-e hâjuyeši Fr.: modèle d'accrétion compétitive A scenario for → massive star formation whereby developing → protostars in their natal → molecular clouds compete with each other to gather mass. The protostars → accrete mass with a rate which depends on their location within the protocluster. They use the same reservoir of gas to grow. Therefore those protostars nearest the center, where the potential well is deep, and gas densities are higher, have the highest → accretion rates. The competitive accretion model explains the observational fact that the most massive stars are generally found in cluster cores. It accounts also for the distribution of stellar masses. In this model the accretion process depends on the content of the cluster. In clusters where gas dominates the potential (e.g. at initial stages of cluster formation), the accretion process is better modeled by using the → tidal radius as the accretion radius. In contrast, when the stars dominate the cluster potential and are virialized, the accretion is better modeled by → Bondi-Hoyle accretion (Bonnell et al. 1997, MNRAS 285, 201; 2001, MNRAS 323, 785). → competitive; → accretion; → model. |
compilation hâtaleš Fr.: compilation The act of compiling; something compiled. |
complex conjugate hamyuq-e hamtâft (#) Fr.: conjugé A → complex number in which the → real part of the number remains the same, but i is replaced by -i. For example, the complex conjugate of x + iy is x - iy. Same as → conjugate complex number. |
complex fraction barxe-ye hamtâft Fr.: fraction complexe A fraction in which the → numerator or → denominator, or both, contain fractions. For example (3/5)/(6/7). Also called → compound fraction. |
complex function karyâ-ye hamtâft Fr.: fonction complexe A function whose → variables are → complex numbers. |
complex population porineš-e hamtâft Fr.: population complexe Same as → composite population. → complex; → population. |
component hamneh (#) Fr.: composante A constituent part; an individual part of an organized whole. L. componentem, pr.p. of componere "to put together," → compose. Hamneh from ham- "together," → com- + neh present tense stem of nehâdan "to put, place," → compose. |
composite population porineš-e hamnehâdé Fr.: population composite A stellar population consisting of more than one → simple population. Also called complex population. → composite; → population. |
composition hamneheš (#) Fr.: composition 1) General: The act or manner of composing; the result or product of composing. Hamnehesh, from ham-, → com-, + neheš verbal noun from nehâdan "to put, place," → compose. |
compound fraction barxe-ye hamnât Fr.: fraction composée Same as → complex fraction. |
compound proposition gozâre-ye hamnât Fr.: proposition composée A statement formed from simple statements by the use of words such as "and," "or," "not," "implies," or their corresponding symbols. → compound; → proposition. |
comprehension hamnuteš Fr.: compréhension 1) The ability to → comprehend
something. Verbal noun of → comprehend. |
compression tanješ (#) Fr.: compression The act or process of compressing; the state of being compressed. Verbal noun from → compress. |
compression factor karvand-e tanješ Fr.: facteur de compression In thermodynamics, the quantity Z = pVm/RT, in which P is the gas pressure, Vm the molar volume, R the gas constant, and T the temperature. The compression factor is a measure of the deviation of a real gas from an ideal gas. For an ideal gas the compression factor is equal to 1. → compression; → facteur. |
compression wave mowj-e tanješ Fr.: onde de compression A → longitudinal wave that compresses the → medium along the direction of → propagation, such as a → sound wave. Same as → compressional wave. → compression; → wave. |
compressional tanješi (#) Fr.: de compression Of or relating to → compression. → compression; → -al. |
compressional wave mowj-e tanješi Fr.: onde de compression An → elastic wave that travels through a → medium with the particles of the medium moving in the same direction as the wave propagation. The compressional wave is the wave that is primarily used in → seismic exploration. Also called P-wave, primary wave, pressure wave. → compressional; → wave. |
Compton Compton Fr.: Compton The American physicist Arthur Holly Compton (1892-1962),
the Nobel Prize in Physics 1927, who made important contributions
to the study of X- and cosmic rays. |
<< < "no abe acc act aff ama ani ant aps ast atm aut bar bic Boh bou cal car cel che cla col com com Com con con con con con con con con con con con con Cor cor cot cul de- dec dem des dif dil dir dis dom dyn Edd ele ele emi equ Eve exc exp fac fin for fre fuz gen Glo gra gra Ham hel hor hyd ign inc inf Inf int Int int ion irr jum Lag lea lig lin Lor Lyo mag mat met min Mon moo NaC neg New New non non non nul obs one opt Ori oxi par per per phl pho pla Pla pol pos pre pro pro pse qua rad rad rea rec reg rel res ret rot Ryd sci sec sec seq sim Sod sor spe sta ste sto sub sup syn the Tho Tor tra tru und vec vio wav Wil zir > >>