éîæïòíáãéïîîùê âàììåôåîø "óôáôøé" N 40.          19.10.98


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          ó 15 ôåïòéñ ÷åòïñôîïóôåê é íáôåíáôéþåóëáñ óôáôéóôéëá

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          ó 322.1 ïâýáñ ôåïòéñ ïôîïóéôåìøîïóôé é çòá÷éôáãéñ

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          ó 322.2 ëïóíïìïçéñ.çòá÷éôáãéïîîùå ÷ïìîù

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    54. Coccia E. a.o.   Hollow Sphere as a Detector of
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    56. Durrer R., Kunz M. Cosmic Microwave Background Anisotropies
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    64. Hu W. a.o.   Complete Treatment of CMB Anisotropies in a FRW
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    66. Iguchi O. a.o.   Renormalization Group Approach to the
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    68. Levin Yu. Quantum Nondemolition and Higher Order Effects for
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          ó 322.4 ë÷áîôï÷áñ çòá÷éôáãéñ

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          ó 323 ë÷áîôï÷áñ íåèáîéëá

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          ó 323.1 òåìñôé÷éóôóëéå ÷ïìîï÷ùå õòá÷îåîéñ. õòá÷îåîéñ ôéðá
âåôå-óïìðéôåòá.ë÷áúéðïôåîãéáì.

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          ó 324.1Á ë÷áîôï÷áñ üìåëôòïäéîáíéëá.üëóðåòéíåîôù ðï
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          ó 324.1 óéìøîùå ÷úáéíïäåêóô÷éñ.üìåëôòïíáçîéôîáñ óôòõëôõòá
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          ó 324.1× óìáâùå ÷úáéíïäåêóô÷éñ.ôåïòéñ ÷áêîâåòçá-óáìáíá é
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          ó 324.1Ç1 ëáìéâòï÷ïþîùå ðïìñ îá òåûåôëå

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          ó 324.1Ä ë÷áîôï÷áñ èòïíïäéîáíéëá

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          ó 324.1Å óõðåòóéííåôòéþîùå ôåïòéé. óõðåòçòá÷éôáãéñ.
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          ó 347 ëïóíéþåóëéå ìõþé

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          ó 393 Ú1 ïòçáîéþåóëéå ó÷åòèðòï÷ïäîéëé é ó÷åòèðòï÷ïäîéëé ó
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          ó 393 É ÷ùóïëïôåíðåòáôõòîáñ ó÷åòèðòï÷ïäéíïóôø.îï÷ùå ÷ôóð

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          ó 393 É1 óôòõëôõòîùå éóóìåäï÷áîéñ.

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    341. O'Connor J.D. a.o.   The Transmission Electron Microscopy
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          ó 393 É2 üìåëôòïíáçîéôîùå é ïðôéþåóëéå ó÷ïêóô÷á.

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    351. Kopf A., Raffelt G. Photon Dispersion in a Supernova Core.
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          ã 840 ðòïçòáííéòï÷áîéå. ïâýéå ÷ïðòïóù

    352. ëÏÒÏÌÅ× ì. ï ËÏÍÐØÀÔÅÒÎÙÈ ÐÒÏÆÅÓÓÉÑÈ.ëÏÍÐÏÚÉÔÏÒÙ
ËÏÍÐØÀÔÅÒÎÏÇÏ ÍÉÒÁ. //îÁÕËÁ É ÖÉÚÎØ. - 1998.- N.9.  - Ó.74-79.


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