ìÇÏïáñ гٵ³ñÓáõÙÛ³ÝÇ Ï³ñ¨áñ³·áõÛÝ ·Çï³Ï³Ý ³ñ¹ÛáõÝùÝ»ñÁ (by H.A. Harutyunian and A.M. Mickaelian)

Eng    Rus

 

 

1. ²é³çÇÝ ³Ý·³Ù ë»÷³Ï³Ý ³ñÅ»ùÝ»ñÇÝ Ñ³Ù³å³ï³ë˳ÝáÕ ¹Çý»ñ»ÝóÇ³É Ñ³í³ë³ñÙ³Ý ï»ëùÁ ·ïÝ»Éáõ ÷áñÓ ¿ ³ñí»É: ²é³çÇÝ ³Ý·³Ù Ó¨³Ï»ñåí»É ¿ ÞïáõñÙ-ÈÇáõíÇÉÇ ËݹñÇÝ Ñ³Ï³¹³ñÓ ËݹÇñ, áñÁ ѻﳷ³ÛáõÙ ¹³ñÓ³í ÝٳݳïÇå ѳϳ¹³ñÓ ËݹÇñÝ»ñÇ Ñ»ï³½áïáõÃÛ³Ý ÙÇ ³ÙµáÕç áõÕÕáõÃÛ³Ý ëÏǽµ (1929 Ã.):
   •   W.A. Ambarzumjan – Uber eine Frage der Eigenwerttheorie (On a Problem of the Theory of Eigenvalues) // Zeitschrift fur Physik, Vol. 53, Nos. 9-10, p. 690-695, 1929 (in German).
   

 

2. ²é³ç ¿ ù³ßí»É ·³Õ³÷³ñ, Áëï áñÇ áã ÙdzÛÝ ¿É»Ïïñ³Ù³·ÝÇë³Ï³Ý ¹³ßïÇ ùí³ÝïÝ»ñÁ` ýáïáÝÝ»ñÁ, ³Ûɨ ÙÛáõë Ù³ëÝÇÏÝ»ñÁ (³Û¹ Ãíáõ٠ѳݷëïÇ áã ½ñáÛ³Ï³Ý ½³Ý·í³Í áõÝ»óáÕÝ»ñÁ) ϳñáÕ »Ý ÍÝí»É ¨ áãÝã³Ý³É ³ÛÉ Ù³ëÝÇÏÝ»ñÇ Ñ»ï ÷á˳½¹»óáõÃÛ³Ý Ñ»ï¨³Ýùáí (³Û¹ ·³Õ³÷³ñÝ ÁÝÏ³Í ¿ ï³ññ³Ï³Ý Ù³ëÝÇÏÝ»ñÇ Å³Ù³Ý³Ï³ÏÇó ýǽÇϳÛÇ ¨ ¹³ßïÇ ùí³Ýï³ÛÇÝ ï»ëáõÃÛ³Ý ÑÇÙùáõÙ) (¸.¸. Æí³Ý»ÝÏáÛÇ Ñ»ï ѳٳï»Õ, 1930 Ã.):
   W.A. Ambarzumjan, D.D. Iwanenko – Eine quantentheoretische Bemerkung zur einheitlichen Feldtheorie (A Quantum-Theoretical Remark on the Uniform Field Theory) // Äîêëàäû Àêàäåìèè Íàóê ÑÑÑÐ, ñåð. À (Doklady USSR Acad. Sci., Ser. A), Vol. 3, p. 45-49, 1930 (in German).
   

 

3. ²å³óáõó»É ¿ ³ïáÙ³ÛÇÝ ÙÇçáõÏÝ»ñáõÙ ³½³ï ¿É»ÏïñáÝÝ»ñÇ ·áÛáõÃÛ³Ý ³ÝÑݳñÇÝáõÃÛáõÝÁ: òáõÛó ¿ ïñí»É, áñ µ³óÇ åñáïáÝÝ»ñÇó ÙÇçáõÏÝ»ñáõ٠ϳñáÕ »Ý ÉÇÝ»É ·ñ»Ã» ÝáõÛÝ ½³Ý·í³ÍÇ ¿É»Ïïñ³ã»½áù Ù³ëÝÇÏÝ»ñ: ¸ñ³ÝÇó »ñÏáõ ï³ñÇ ³Ýó æ»ÛÙë ⻹íÇÏÁ ѳÛïݳ·áñÍ»ó Ý»ÛïñáÝÁ (¸.¸. Æí³Ý»ÝÏáÛÇ Ñ»ï ѳٳï»Õ,1930 Ã.):
   •  W.A. Ambarzumjan, D.D. Iwanenko – Uber eine Folgerung der Diracschen Theorie der Protonen und Elektronen (On a Consequence of the Dirac Theory of Protons and Electrons) // Äîêëàäû Àêàäåìèè Íàóê ÑÑÑÐ, ñåð. À (Doklady USSR Acad. Sci., Ser. A), Vol. 6, p. 153-155, 1930 (in German).
   V.A. Ambartsoumian, D.D. Ivanenko – Les electrons inobservables et les rayons β (The Inobservable Electrons and β Rays) // Compte rendu hebdomadaire des seances de l'Academie des sciences de Paris, Vol. 190, No. 9, p. 582-584, 1930 (in French).
   

 

4. ²é³çÇÝ ³Ý·³Ù ѻﳽáïí»É ¿ Ï»ÝïñáÝ³Ï³Ý ³ëïÕÇ ÉáõÛëÇ ×ÝßÙ³Ý ³½¹»óáõÃÛ³Ý ï³Ï ÙáÉáñ³Ï³Ó¨ ÙÇ·³Ù³ÍáõÃÛáõÝÝ»ñÇ É³ÛݳóÙ³Ý Ù»Ë³ÝǽÙÁ: òáõÛó ¿ ïñí»É, áñ ÉáõÛëÇ ×ÝßÙ³Ý Ñ»ï¨³Ýùáí ³Û¹ ÙÇ·³Ù³ÍáõÃÛáõÝÝ»ñÁ ɳÛݳÝáõÙ ¨ óñíáõÙ »Ý ï³ñ³ÍáõÃÛ³Ý Ù»ç ¨ áñ ¹ñ³Ýù ã»Ý ϳñáÕ ·áÛ³ï¨»É 100000 ï³ñáõó ³í»ÉÇ, »Ã» ³ëïÕÇó ³ÝÁÝ¹Ñ³ï ³ñï³Ñáëù ãϳ: ²é³çÇÝ ³Ý·³Ù Ó¨³íáñí»É ¿ ïÇ»½»ñ³Ï³Ý ³í»ÉÇ ËÇï ÝÛáõÃÇó ³í»ÉÇ Ýáëñ ûµÛ»ÏïÝ»ñÇ ³é³ç³óÙ³Ý å³ñ³¹Ç·ÙÁ (1932 Ã.):
   •  V.A. Ambartsumian – The Radiative Equilibrium of a Planetary Nebula // Monthly Notices of the Royal Astronomical Society (MNRAS), Vol. 93, No. 1, p. 50-61, 1932 (in English).
   

 

5. ²é³ç³ñÏ»É ¿ ÙáÉáñ³Ï³Ó¨ ÙÇ·³Ù³ÍáõÃÛáõÝÝ»ñÇ Ï»ÝïñáÝ³Ï³Ý ³ëïÕ»ñÇ Ù³Ï»ñ¨áõóÛÇÝ ç»ñÙ³ëïÇ׳ÝÝ»ñÇ áñáßÙ³Ý Ýáñ »Õ³Ý³Ï (¼³Ýëïñ³ÛÇ »Õ³Ý³ÏÇ ½³ñ·³óáõÙÁ) áõ ïí»É ϳñ׳ÉÇù ýáïáÝÝ»ñÇ í»ñ³÷áËÙ³Ý Ñ³í³Ý³Ï³Ý³ÛÇÝ Ó¨³Ï»ñåáõÙÁ, áñÁ ѳݷ»óÝáõÙ ¿ ÙáÉáñ³Ï³ÛÇÝ ÙÇ·³Ù³ÍáõÃÛáõÝÝ»ñÇ ×³é³·³ÛóÛÇÝ Ñ³í³ë³ñ³ÏßéáõÃÛ³Ý ë³ÑÙ³ÝÙ³ÝÁ (1932 Ã.):
   •  V.A. Ambartsumian – On the Temperatures of the Nuclei of Planetary Nebulae // Öèðêóÿð Ïóëêîâñêîé Îáñåðâàòîðèè (Poulkovo Observatory Circular), No. 4, p. 8-12, 1932 (in English).
   

 

6. ²é³çÇÝ ³Ý·³Ù ·Ý³Ñ³ïí»É »Ý Üáñ ¨ ¶»ñÝáñ ³ëïÕ»ñÇ ÏáÕÙÇó ³ñï³Ý»ïíáÕ ÝÛáõÃÇ ù³Ý³ÏÁ ¨ óճÝÃÝ»ñÇ ½³Ý·í³ÍÝ»ñÁ: êï³óí»É ¿ ÙÇÝ㨠ûñë û·ï³·áñÍíáÕ ·Ý³Ñ³ï³Ï³ÝÁ, Áëï áñÇ ÜáñÇ µéÝÏÙ³Ý Å³Ù³Ý³Ï ³ñï³Ý»ïíáõÙ ¿ 0.00001 ²ñ»·³ÏÇ ½³Ý·í³Íáí, ÇëÏ ¶»ñÝáñ»ñÁ ¹áõñë »Ý ßåñïáõÙ ²ñ»·³ÏÇ Ù»Ï ½³Ý·í³ÍÇÝ Ñ³í³ë³ñ ÝÛáõà (Ü.². Îá½Çñ¨Ç Ñ»ï ѳٳï»Õ, 1933 Ã.):
   •  W.A. Ambarzumjan, N.A. Kosyrew – Uber die Massen der von den neuen Sternen ausgestossenen Gashullen (On the Masses of Envelopes thrown out by Novae) // Zeitschrift fur Astrophysik, Vol. 7, No. 4, p. 320-325, 1933 (in German).
   

 

7. ²ëïÕ»ñÇ ï»ë³·Í³ÛÇÝ ³ñ³·áõÃÛáõÝÝ»ñÇ ¨ »ñÏݳÛÇÝ Ïááñ¹ÇݳïÝ»ñÇ ÙÇçáóáí ³é³çÇÝ ³Ý·³Ù ³ñï³Íí»É ¿ Ýñ³Ýó ï³ñ³Í³Ï³Ý ³ñ³·áõÃÛáõÝÝ»ñÇ µ³ßËÙ³Ý ýáõÝÏódzÝ, áñÁ ѳݷ»óí»É ¿ñ è³¹áÝÇ Ñ³Ï³¹³ñÓ Ó¨³÷áËáõÃÛáõÝ Ï³ï³ñ»ÉáõÝ: âáñë ï³ëݳÙÛ³Ï ³Ýó ³Û¹ ÝáõÛÝ Ù³Ã»Ù³ïÇÏ³Ï³Ý ³å³ñ³ïÁ ÏÇñ³éí»ó ïáÙá·ñ³ýÝ»ñÇ ëï»ÕÍÙ³Ý ¨ ߳ѳ·áñÍÙ³Ý Ýå³ï³Ïáí (1936 Ã.):
   •  V.A. Ambartsumian – On the Derivation of the Frequency Function of Space Velocities of the Stars from the Observed Radial Velocities // Monthly Notices of the Royal Astronomical Society (MNRAS), Vol. 96, No. 3, p. 172-179, 1936 (in English).
   

 

8. ò³Íñ ·³É³ÏïÇÏ³Ï³Ý É³ÛÝáõÃÛáõÝÝ»ñáõÙ ëåÇï³Ï ³ëïÕ»ñÇ áõëáõÙݳëÇñáõÃÛ³Ý ÙÇçáóáí óáõÛó ¿ ïñí»É ëåÇï³Ï ýáõÏ ³ëïÕ»ñÇ µ³½Ù³ù³Ý³ÏáõÃÛáõÝÁ ¶³É³ÏïÇϳÛáõÙ, ÇÝãÁ ѻﳷ³ÛáõÙ ³å³óáõóí»ó Ù»Í Ãíáí ëåÇï³Ï ýáõÏÝ»ñÇ Ñ³Ûïݳµ»ñٳٵ (¶.². Þ³ÛÝÇ Ñ»ï ѳٳï»Õ, 1936 Ã.):
   •  V.A. Ambartsumian, G.A. Shain – On the Faint White Stars in Low Galactic Latitudes // Àñòðîíîìè÷åñêèé Æóðíàë (Soviet Astronomy), Vol. 13, No. 1, p. 1-7, 1936 (in English).
   

 

9. ȳÛÝ ³ëïÕ³½áõÛ·»ñÇ íÇ׳ϳ·ñ³Ï³Ý ѻﳽáïáõÃÛ³Ùµ ³é³çÇÝ ³Ý·³Ù óáõÛó ¿ ïñí»É, áñ ¹ñ³Ýù Ñ»éáõ »Ý ¹ÇëáódzïÇí ѳí³ë³ñ³ÏßéáõÃÛáõÝÇó: ¸³ ÃáõÛÉ ¿ ïí»É ³å³óáõó»É, áñ ³ëïÕ³½áõÛ·»ñÇ µ³Õ³¹ñÇãÝ»ñÝ ³é³ç³ó»É »Ý ѳٳï»Õ ¨ áñ ¹ÇïíáÕ µ³ßËáõÙÁ í»ñÇÝ ë³ÑÙ³Ý ¿ ¹ÝáõÙ ¶³É³ÏïÇϳÛÇ ï³ñÇùÇ íñ³` 10 ÙÉñ¹ ï³ñÇ: ¸ñ³Ýáí ³å³óáõó»É ¿ ¶³É³ÏïÇϳÛÇ ï³ñÇùÇ ÙÇÝã ³Û¹ ·»ñÇßËáÕ æ»ÛÙë æÇÝëÇ ·Ý³Ñ³ï³Ï³ÝÇ (§Å³Ù³Ý³ÏÇ »ñϳñ ë³Ý¹Õ³ÏǦ` 10¹³ ï³ñÇ) ëË³É ÉÇÝ»ÉÁ ¨ ³å³óáõó»É §Å³Ù³Ý³ÏÇ Ï³ñ× ë³Ý¹Õ³ÏǦ ×ßÙ³ñï³óÇáõÃÛáõÝÁ (1936-1937 ÃÃ.):
   •  V.A. Ambartsumian – Double Stars and the Cosmogonic Time-Scale // Nature, Vol. 137, No. 3465, p. 537, 1936 (in English).
   •  Â.À. Àìáàðöóìÿí – Ê ñòàòèñòèêå äâîéíûõ çâåçä (On the Statistics of Double Stars) // Àñòðîíîìè÷åñêèé Æóðíàë (Astron. Zh.), Vol. 14, No. 3, p. 207-219, 1937 (in Russian).
   

 

10. ²ëïÕ³ÛÇÝ Ñ³Ù³Ï³ñ·»ñÇ íÇ׳ϳ·ñ³Ï³Ý ٻ˳ÝÇϳÛÇ ÑÇÙáõÝùÝ»ñÁ: ´³ó³Ñ³Ûïí»É ¿ µ³ó ³ëïÕ³ÏáõÛï»ñÇ §·áÉáñß³óٳݦ ٻ˳ÝǽÙÁ, ÇÝãÁ ÃáõÛÉ ¿ ïí»É ³é³çÇÝ ³Ý·³Ù ·Ý³Ñ³ï»É ¹ñ³Ýó ÏÇë³ïñáÑÙ³Ý å³ñµ»ñáõÃÛáõÝÁ (óáõÛó ¿ ïñí»É, áñ ³ëïÕ³ÏáõÛï»ñÁ ïñáÑíáõÙ »Ý 1 ÙÉñ¹ ï³ñí³ ÁÝóóùáõÙ), ϳÝ˳·áõß³Ï»É Ã½áõÏ ³ëïÕ»ñáí ³ëïÕ³ÏáõÛï»ñÇ ³Õù³ï³óÙ³Ý åñáó»ëÁ: ²Ûë ѻﳽáïáõÃÛáõÝÁ ³ÛÝ ÑÇÙù»ñÇó Ù»ÏÝ ¿ñ, áñ ÃáõÛÉ ïí»ó ¶³É³ÏïÇϳÛÇ ÁݹáõÝí³Í ï³ñÇùÁ å³Ï³ë»óÝ»É »ñ»ù ϳñ·áí ¨ ·áñͳÍáõÃÛ³Ý Ù»ç ¹Ý»É ¶³É³ÏïÇϳÛÇ ï³ñÇùÇ §Ï³ñ× ë³Ý¹Õ³ÏÁ¦ (1938 Ã.):
    •  Â.À. Àìáàðöóìÿí – Ê âîïðîñó î äèíàìèêå îòêðûòûõ ñêîïëåíèé (On the Dynamics of Open Clusters) // Òðóäû ÀÎ ËÃÓ; Ó÷. çàï. ËÃÓ, Ñåðèÿ ìàò. íàóê (Àñòðîíîìèÿ), âûï. 4 (Trudy LGU; Ucheniye Zapiski LGU, Ser. Math. Sciences (Astronomy). Issue 4), No. 22, p. 19-22, 1938 (in Russian).
    

 

11. ØÇç³ëïÕ³ÛÇÝ ÏɳÝáÕ ÝÛáõÃÇ (ÌÇñ γÃÝÇ ÷áß³ÛÇÝ µ³Õ³¹ñÇãÇ) µÝáõÛÃÇ ¨ å³ï³é³Ó¨ ϳéáõóí³ÍùÇ µ³ó³Ñ³ÛïáõÙÝ áõ ³é³ÝÓÇÝ ³Ùå»ñÇ ÏɳÝÙ³Ý ÙÇçÇÝ ã³÷Ç ·Ý³Ñ³ïáõÙÁ: ²é³çÇÝ ³Ý·³Ù óáõÛó ïñí»ó, áñ ³Û¹ ³Ùå»ñÁ ÙÇçÇÝáõÙ ÏɳÝáõÙ »Ý 0.2 ³ëïÕ³ÛÇÝ Ù»ÍáõÃÛ³Ý ã³÷áí (Þ.¶. ¶áñ¹»É³Ó»Ç Ñ»ï ѳٳï»Õ, 1938 Ã.):
    •  V.A. Ambartsumian, Sh.G. Gordeladze – Problem of Diffuse Nebulae and Cosmic Absorption // Áþëëåòåíü Àáàñòóìàíñêîé ÀÎ (Bulletin of the Abastumani Astrophysical Observatory), No. 2, p. 37-68, 1938 (in English and Georgian).
    

 

12. äÕïáñ ÙÇç³í³ÛñáõÙ ÉáõÛëÇ óñÙ³Ý Ýáñ ï»ëáõÃÛ³Ý` ÆÝí³ñdzÝïáõÃÛ³Ý ï»ëáõÃÛ³Ý, Ùß³ÏáõÙÁ: ֳ鳷³ÛÃÙ³Ý ï»Õ³÷áËÙ³Ý ËݹÇñÝ»ñÇ ÉáõÍÙ³Ý Ýå³ï³Ïáí ³é³ç³ñÏ»É ¿ ÆÝí³ñdzÝïáõÃÛ³Ý ëϽµáõÝù: ²ÛÝ å³ñ½ ýǽÇÏ³Ï³Ý ¹³ïáÕáõÃÛáõÝÁ, áñ ÏÇë³³Ýí»ñç ѳñÃ-½áõ·³Ñ»é ÙÇç³í³ÛñÇÝ ÝáõÛÝ Ñ³ïÏáõÃÛáõÝÝ»ñáí µ³ñ³Ï ß»ñïÇ ³í»É³óáõÙÁ ãÇ ÷áËáõÙ Ýñ³ ³Ý¹ñ³¹³ñÓÙ³Ý Ñ³ïÏáõÃÛáõÝÝ»ñÁ, ÑÇÙù ѳݹÇë³ó³í ѻﳽáï³Ï³Ý Ýáñ Ùáï»óÙ³Ý ëï»ÕÍÙ³Ý Ñ³Ù³ñ (1941-1942 ÃÃ.):
    •  Â.À. Àìáàðöóìÿí – Íîâûé ñïîñîá ðàñ÷åòà ðàññåÿíèÿ ñâåòà â ìóòíîé ñðåäå (A New Method of Calculation of the Light Scattering in Turbid Medium) // Èçâåñòèÿ ÀÍ ÑÑÑÐ, ñåðèÿ ãåîãðàôè÷åñêàÿ è ãåîôèçè÷åñêàÿ (Izvestiya Acad. Sci. USSR, Ser. Geograph. and Geophys. Sci.), Vol. 3, p. 97-103, 1942 (in Russian).
    V.A. Ambartsumian – The Scattering of Light in a Turbid Medium // Journal of Physics, Vol. 5, No. 1, p. 93, 1941 (in English).
    

 

13. ÌÇñ γÃÝÇ å³ÛͳéáõÃÛ³Ý ýÉáõÏïáõ³ódzݻñÇ ï»ëáõÃÛáõÝÁ, áñÁ ϳñáÕ ¿ ë³ÑÙ³Ýí»É ß³ï å³ñ½ Ó¨³Ï»ñåٳٵ` ³Ýí»ñç ûåïÇÏ³Ï³Ý Ñ³ëïáõÃÛ³Ý ë³ÑٳݳÛÇÝ ¹»åùáõÙ ÌÇñ γÃÝÇ å³ÛͳéáõÃÛ³Ý ýÉáõÏïáõ³ódzݻñÇ µ³ßËáõÙÝ ÇÝí³ñdzÝï ¿ ¹ÇïáÕÇ ¹ÇñùÇ Ýϳïٳٵ (1944 Ã.):
    •  Â.À. Àìáàðöóìÿí – Ê òåîðèè ôëþêòóàöèè ÿðêîñòè Ìëå÷íîãî Ïóòè (To the Theory of Fluctuation in the Brightness of the Milky Way) // Äîêëàäû Àêàäåìèè Íàóê ÑÑÑÐ (Doklady USSR Acad. Sci.), Vol. 44, No. 6, p. 244-247, 1944 (in Russian).
    

 

14. ²ëïÕ³ë÷ÛáõéÝ»ñÇ` ç»ñÙ ÑëϳݻñÇ ¨ T òáõÉÇ ïÇåÇ ³ëïÕ»ñÇ ËÙµ³íáñáõÙÝ»ñÇ, ѳÛïݳ·áñÍáõÙÁ: ²é³çÇÝ ³Ý·³Ù óáõÛó ïñí»ó, áñ ³ëïÕ»ñÝ ³é³ç³ÝáõÙ »Ý ¶³É³ÏïÇϳÛÇ ¿íáÉÛáõódzÛÇ µáÉáñ ÷áõÉ»ñáõÙ, ³Û¹ Ãíáõ٠ݳ¨ Ý»ñϳÛáõÙë, ¨ áñ ³ëïÕ³é³ç³óáõÙÝ ³ÝÁݹѳï åñáó»ë ¿: òáõÛó ïñí»ó, áñ ³ëïÕ»ñÝ ³é³ç³ÝáõÙ »Ý áã û ³é³ÝÓÇÝ-³é³ÝÓÇÝ, ³ÛÉ` ËÙµ»ñáí (1947 Ã.):
    •  Evolution of Stars and Astrophysics // Acad. Sci. ArmSSR, 39 p., Yerevan, 1948 (in Armenian).
    •  Â.À. Àìáàðöóìÿí – Ïðåäâàðèòåëüíûå äàííûå îá Î-àññîöèàöèÿõ â Ãàëàêòèêå (Preliminary Data on O-Associations in the Galaxy) // Äîêëàäû Àêàäåìèè Íàóê ÑÑÑÐ (Doklady USSR Acad. Sci.), Vol. 68, No. 1, p. 21-22, 1949 (in Russian).
    

 

15. ²ëïÕ³ë÷ÛáõéÝ»ñÇ Áݹ³ñÓ³ÏÙ³Ý »ñ¨áõÛÃÇ ï»ë³Ï³Ý ϳÝ˳·áõß³ÏáõÙÁ: úñÇáÝÇ îñ³å»ódzÛÇ ïÇåÇ Ñ³Ù³Ï³ñ·»ñÇ íÇ׳ϳ·ñáõÃÛáõÝÁ ¨ »ñÇï³ë³ñ¹ ³ëïÕ³ÛÇÝ Ñ³Ù³Ï³ñ·»ñÇ ù³Ûù³ÛÙ³Ý ³å³óáõÛóÁ (´.º. سñ·³ñÛ³ÝÇ Ñ»ï ѳٳï»Õ, 1949-1951 ÃÃ.):
    •  Â.À. Àìáàðöóìÿí – Çâåçäíûå àññîöèàöèè (Stellar Associations) // Àñòðîíîìè÷åñêèé Æóðíàë (Astron. Zh.), Vol. 26, No. 1, p. 3-9, 1949 (in Russian).
    •  Â.À. Àìáàðöóìÿí, Á.Å. Ìàðêàðÿí (V.A. Ambartsumian, B.E. Markarian) – Çâåçäíàÿ àññîöèàöèÿ âîêðóã Ð Ëåáåäÿ (Stellar Association around P Cygni) // Ñîîáùåíèÿ Áþðàêàíñêîé îáñåðâàòîðèè (Communications of the Byurakan Observatory), No. 2, p. 3-17, 1949 (in Russian).
    •  Â.À. Àìáàðöóìÿí – Î âåðîÿòíîñòè êàæóùèõñÿ êðàòíûõ ñèñòåì òèïà Òðàïåöèè Îðèîíà (On the Frequency of the Orion Trapezium type Apparent Multiple Systems) // Äîêëàäû Àêàäåìèè Íàóê ÀðìÑÑÐ (Doklady Acad. Sci. ArmSSR), Vol. 13, No. 4, p. 97-103, 1951 (in Russian).
    •  Â.À. Àìáàðöóìÿí – Ê ñòàòèñòèêå êðàòíûõ ñèñòåì òèïà Òðàïåöèè (On the Statistics of Trapezium type Multiple Systems) // Äîêëàäû Àêàäåìèè Íàóê ÀðìÑÑÐ (Doklady Acad. Sci. ArmSSR), Vol. 13, No. 5, p. 129-131, 1951 (in Russian).
    

 

16. ²å³óáõó»É ¿ ³ÝϳÛáõÝ ³ëïÕ»ñÇ ëå»ÏïñÝ»ñáõÙ ¹ÇïíáÕ ³ÝÁÝ¹Ñ³ï ³é³ùÙ³Ý áã ç»ñÙ³ÛÇÝ µÝáõÛÃÁ ¨ ³é³ç ¿ ù³ß»É ·³Õ³÷³ñ ³ëïÕ³ÛÇÝ ×³é³·³ÛÃÙ³Ý ¿Ý»ñ·Ç³ÛÇ Ýáñ Ñݳñ³íáñ ³ÕµÛáõñÝ»ñÇ í»ñ³µ»ñÛ³É` ݳ˳ëïÕ³ÛÇÝ ·»ñËÇï ÝÛáõÃÇ Ù³ëÇÝ í³ñϳÍÁ (1954 Ã.):
    •  Â.À. Àìáàðöóìÿí – ßâëåíèå íåïðåðûâíîé ýìèññèè è èñòî÷íèêè çâåçäíîé ýíåðãèè (The Phenomenon of the Continuous Emission and Sources of Stellar Energy) // Ñîîáùåíèÿ Áþðàêàíñêîé îáñåðâàòîðèè (Communications of the Byurakan Observatory), No. 13, p. 1-36, 1954 (in Russian).
    

 

17. ¶³É³ÏïÇϳݻñÇ ÙÇçáõÏÝ»ñÇ ³ÏïÇíáõÃÛ³Ý ·³Õ³÷³ñÁ: ²é³çÇÝ ³Ý·³Ù áõß³¹ñáõÃÛáõÝ Ññ³íÇñí»ó ³ÏïÇíáõÃÛ³Ý ï³ñµ»ñ Ó¨»ñÇÝ, ¹ñ³Ýù Ù»Ïݳµ³Ý»Éáí ǵñ¨ ÙÇçáõÏÇ ýǽÇÏ³Ï³Ý ³ÏïÇíáõÃÛ³Ý »ñ¨áõÛÃÇ ï³ñµ»ñ ¹ñë¨áñáõÙÝ»ñ: òáõÛó ïñí»ó ·³É³ÏïÇϳݻñÇ ÙÇçáõÏÝ»ñÇ ³ÏïÇíáõÃÛ³Ý ¿íáÉÛáõóÇáÝ Ý߳ݳÏáõÃÛáõÝÁ ¨ ³é³ç³ñÏí»ó í³ñÏ³Í ÙÇçáõÏÝ»ñÇ ³ÏïÇíáõÃÛ³Ý ßÝáñÑÇí Ýáñ ·³É³ÏïÇϳݻñÇ ÍÝÙ³Ý í»ñ³µ»ñÛ³É: Üáñ ½³ñ·³óáõÙ ëï³ó³í ݳ˳ëïÕ³ÛÇÝ ·»ñËÇï ÝÛáõÃÇ í»ñ³µ»ñÛ³É í³ñϳÍÁ (1956 Ã.):
    •  Â.À. Àìáàðöóìÿí – Ê âîïðîñó î ïðèðîäå èñòî÷íèêîâ ðàäèîèçëó÷åíèÿ (On the Nature of Radio Sources) // Òðóäû Ïÿòîãî ñîâåùàíèÿ ïî âîïðîñàì êîñìîãîíèè: "Ðàäèîàñòðîíîìèÿ", 9-12 ìàðòà 1955 ã., ÀÍ ÑÑÑÐ (Proc. Fifth conference on Problems of Cosmogony: "Radioastronomy", held on 9-12 Mar 1955. Acad. Sci. USSR), p. 413-416, Ìîñêâà (Moscow), 1956 (in Russian).
    •  Â.À. Àìáàðöóìÿí – Î êðàòíûõ ãàëàêòèêàõ (On Multiple Galaxies) // Èçâåñòèÿ ÀÍ ÀðìÑÑÐ, ñåðèÿ ôèçèêî-ìàòåìàòè÷åñêèõ, åñòåñòâåííûõ è òåõíè÷åñêèõ íàóê (Izvestiya Acad. Sci. ArmSSR, Ser. Phys.-Math., Nat. and Tech. Sci.), Vol. 9, No. 1, p. 23-43, 1956 (in Russian).
    

 

18. ¶»ñËÇï ³Ûɳë»ñí³Í ³ëïÕ³ÛÇÝ ÏáÝýÇ·áõñ³ódzݻñÇ ï»ë³Ï³Ý ѻﳽáïáõÃÛáõÝÁ. µ³ñÇáݳÛÇÝ ³ëïÕ»ñÇ ï»ëáõÃÛ³Ý ÑÇÙáõÝùÝ»ñÇ Ùß³ÏáõÙÁ, áñÁ ѻﳷ³ÛáõÙ ÃáõÛÉ ïí»ó µ³ñÓñ³óÝ»É ³ëïÕ³ÛÇÝ ½³Ý·í³ÍÝ»ñÇ Ñ³Ù³ñ â³Ý¹ñ³ë»Ï³ñÇ ëï³ó³Í ë³ÑÙ³ÝÁ (¶.ê. ê³Ñ³ÏÛ³ÝÇ Ñ»ï ѳٳï»Õ, 1960-1961 ÃÃ.):
    •  Â.À. Àìáàðöóìÿí, Ã.Ñ. Ñààêÿí (V.A. Ambartsumian, G.S. Saakyan) – Î âûðîæäåííîì ñâåðõïëîòíîì ãàçå ýëåìåíòàðíûõ ÷àñòèö (The Degenerate Superdense Gas of Elementary Particles) // Àñòðîíîìè÷åñêèé Æóðíàë (Astron. Zh.), Vol. 37, No. 2, p. 193-209, 1960 (in Russian) // English translation in: Soviet Astronomy, Vol. 4, No. 2, p. 187-201, 1960.
    •  Â.À. Àìáàðöóìÿí, Ã.Ñ. Ñààêÿí (V.A. Ambartsumian, G.S. Saakyan) – Î ðàâíîâåñíûõ êîíôèãóðàöèÿõ ñâåðõïëîòíûõ âûðîæäåííûõ ãàçîâûõ ìàññ (On Equilibrium Configurations of Superdense Degenerate Gas Masses) // Àñòðîíîìè÷åñêèé Æóðíàë (Astron. Zh.), Vol. 38, No. 5, p. 785-797, 1961 (in Russian) // English transaltion in: Soviet Astronomy, Vol. 5, No. 5, p. 601-610, 1962.
    •  Â.À. Àìáàðöóìÿí, Ã.Ñ. Ñààêÿí (V.A. Ambartsumian, G.S. Saakyan) – Âíóòðåííîå ñòðîåíèå ãèïåðîííûõ êîíôèãóðàöèé çâ¸çäíûõ ìàññ (Internal Structure of Hyperon Configurations of Stellar Masses) // Àñòðîíîìè÷åñêèé Æóðíàë (Astron. Zh.), Vol. 38, No. 6, p. 1016-1024, 1961 (in Russian) // English transaltion in: Soviet Astronomy, Vol. 5, No. 6, p. 779-784, 1962.
    

 

19. ´éÝÏíáÕ ³ëïÕ»ñÇ íÇ׳ϳ·ñ³Ï³Ý ѻﳽáïáõÃÛáõÝÝ»ñÁ. ³é³ç³ñÏí»ó ³ëïÕ³ÛÇÝ Ñ³Ù³Ï³ñ·áõÙ µéÝÏíáÕ ³ëïÕ»ñÇ ÁݹѳÝáõñ ÃíÇ ·Ý³Ñ³ïÙ³Ý Ù»Ãá¹` ÑÇÙÝí³Í ³Û¹ ѳٳϳñ·áõÙ ³ñ¹»Ý ѳÛïÝÇ µéÝÏíáÕ ³ëïÕ»ñÇ ¹ÇïáõÙÝ»ñÇ íñ³: ²ñ¹ÛáõÝùáõÙ å³ñ½í»ó µéÝÏáõÙ³ÛÇÝ ³ÏïÇíáõÃÛ³Ý ûñÇݳã³÷ µÝáõÛÃÁ ó³Íñ Éáõë³ïíáõÃÛ³Ý ¨ ÷áùñ ½³Ý·í³Íáí áõß ¹³ëÇ ³ëïÕ»ñÇ Ñ³Ù³ñ: ²å³óáõóí»ó, áñ ³Û¹ ¹³ëÇ ³ëïÕ»ñÝ Çñ»Ýó »ñÇï³ë³ñ¹áõÃÛ³Ý í³Õ ÷áõÉ»ñáõÙ ³Ýå³ÛÙ³Ýáñ»Ý ³ÝóÝáõÙ »Ý µéÝÏáõÙ³ÛÇÝ ³ÏïÇíáõÃÛ³Ý ÷áõÉáí (1968 Ã.):
    •  Â.À. Àìáàðöóìÿí – Ê ñòàòèñòèêå âñïûõèâàþùèõ îáúåêòîâ (On the Statistics of Flare Objects) // Òðóäû ñèìïîçèóìà "Çâåçäû. Òóìàííîñòè. Ãàëàêòèêè", ïîñâÿùåííîãî 60-ëåòèþ àêàäåìèêà Â.À. Àìáàðöóìÿíà, Áþðàêàí, 16-19 ñåíòÿáðÿ 1968 ã., ÀÍ ÀðìÑÑÐ (Proc. symp. "Stars, Nebulae, Galaxies", devoted to the 60th anniversary of academician V.A. Ambartsumian, held in Byurakan, 16-19 Sep 1968. Acad. Sci. ArmSSR), p. 283-292, Åðåâàí (Yerevan), 1969 (in Russian).
    

 

20. ´éÝÏíáÕ ³ëïÕ»ñÇ Ñ³Ûïݳµ»ñÙ³Ý Å³Ù³Ý³Ï³·ñáõÃÛ³Ý (³é³çÇÝ µéÝÏáõÙÝ»ñÇ) ¨ ѳëï³ïÙ³Ý (»ñÏñáñ¹ µéÝÏáõÙÝ»ñÇ) ÑÇÙ³Ý íñ³ ïíÛ³É ³ëïÕ³ÛÇÝ Ñ³Ù³Ï³ñ·áõÙ µéÝÏáõÙÝ»ñÇ ÙÇçÇÝ Ñ³×³Ë³Ï³ÝáõÃÛ³Ý µ³ßËÙ³Ý ýáõÝÏódzÛÇ ¹áõñëµ»ñáõÙÁ ѳϳ¹³ñÓ ËݹñÇ »Õ³Ý³Ïáí (1978 Ã.):
    •  Â.À. Àìáàðöóìÿí – Âûâîä ðàñïðåäåëåíèÿ ÷àñòîòû çâ¸çäíûõ âñïûøåê â çâ¸çäíîì àãðåãàòå (Derivation of the frequency function of stellar flares in a star cluster) // Àñòðîôèçèêà (Astrofizika), Vol. 14, No. 3, p. 367-381, 1978 (in Russian) // English translation in: Astrophysics, Vol. 14, No. 3, p. 209-217, 1978.