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No. 3.0OJ<_^iJ$N+]b w Jx.+3&fjK

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1
2

3
4
5

6

7

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60NEH_
2.1 |5O : : : : : : : : : : : : : : : : : : : : : : : : : : : : : 4
2.2 60N)0He/ : : : : : : : : : : : : : : : : : : : : : : : 5/.LNQ0
1U'$ITBjST)@5,b?i9iN)0O
5.1 |MKP9kT)@Y : : : : : : : : : : : : : : : : : : : : 9
5.2 .N\0NzL : : : : : : : : : : : : : : : : : : : : : : : : 11
5.3 iN)0ONN' : : : : : : : : : : : : : : : : : : : : : : : 11
)0OKP9kP.NzL
6.1 1U'$ITBjSNV&N< : : : : : : : : : : : : : : : 12
6.2 P.,z-/39;~|NQw : : : : : : : : : : : : : : : 13
6.3 'N}@ : : : : : : : : : : : : : : : : : : : : : : : : : : : : 14
D5l?dj

2
4

5
6
9

12

14

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1

17

Qw1N<H No. 1 KD$F : : : : : : : : : : : : : : : : 17
Qw1N<H No. 2 KD$F : : : : : : : : : : : : : : : : 17
1N=L9Y : : : : : : : : : : : : : : : : : : : : : : : : : 17T)@YN1L : : : : : : : : : : : : : : : : : : : : : : : : 18

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IH-5lF$k. Krh8?MHJk.
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k. 6jRrcKM(kH, 6jR,E_7F$kLV+i, &&K"lPEO,8~-K0/h&K/-, 6jR,8&K"lPEO,&~-K
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for eKHFV.
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.0,J<}37F$k+rM(kH$&3HO, 1ND%}LN]N)0OHiN)0Or&f9k3HKjv9k. 1Nlg, D%9kax
G1NbtN5O,e^kh&J3H,"lP, )0OH7F//. 1M
K, }L9kaxGbtN5O,/^lP, )0OH7F//. .01N}@NpCrV$?"<5<&(G#sHsJArthur EddingtonKO, .
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5

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4

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6

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N60TBjJvibrational instabilityKG"k. 1N=$,4NH7Fx
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free pathKH$&. =N95NUt,T)@YG"k. T)@YN1LO,
95,N 1 G, @8JIGO 1 ;sAa<Hkv?jINxYG"k+H$&h&K(5lF$k.
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F?Q[}8tOb/, =NOOJ0GOfS*c$H$C?-A,"k.
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btKy(ilkH$&3HGb"k. eGN?Q[}8t,bCHbb/JkNO, 1N=LGO9Y, 5 iY+i 2 |YNOObG, =3GO
wN?Q+3TxO, ?+@+t4-ma<HkxYG"k. 1U'&99

= 2: iN)0O,//!=. =f, IC*H==7F$kNO, .NP~jN
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1,D%}Lr+jV7F$klg, 3&7?T)@Jt,O, >B,.5$uVGl~*K|Mr[}7Fy(, 1,D%K>8?eK|P7
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10

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:rhj7&aw!O, G.awJadiabati approximationKHFPlk.
3Nh&Jaw!GO, .N\0r5k9kNG"k+i, 9YN3HO
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7?0sGTolF$?.
7+7, 1N=La/KJkH, 1N)Y,uvKJj, y(ilF$k.LKfYF, \09k.Nf(,b/Jj, 5O, 9Y, )YNQ=rW;9kKv?CF, 3N.N.lrI&+Qbk+,EWKJCF/k. =3G, M(}rQ97, Gi+i.N\0rM87Fdjr)F>9,W,"C?. 3Nh&Jaw!r, sG.awJnon-adiabati approximationK
HFV.
5.3

iN)0ONN';k2$&8't!-sJSergei A. ZhevakinKO, sG.awrNQ
7F, 1U'$IND%}LN?0r!$7, iN)0OH7FB]K1
U'&9BGk??G.0r}35;k?aKO, eG@1GOL*KT<,GXj&`KhkT)@-bM89k,W,"k3HrX&7? (6).
8't!-sNM(r, ERW;!rQ$F, hj\YK&f7?N,
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KippenhahnKG"k. `iO, OaF1U'&9BGk??G.0,}311

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12

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k$N,trJ7Fe:<_9k?0,O^k. 3l,P.J onve tionKG"k. P.O, gLN.rl$K?VNG, b$T)@Y,|MrWk
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6.2

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1N.0KO, 14N,D%}Lr+jV9M0NQ0HOLK, 1N=
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N=L,4t1~Ke,C?j<,C?j9kh&JQ0r, 0B}~6
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@[GO;~|Ns0B}~60,Q,5lF$k,, =N6xO, P.XNfNT,'J$NN0-,z-/39H0,, @[rl~7FzY&67"&h&Jror~?7?lgK, o~Q,5lkQ07F8-D
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3Nh&JaxGz-/35l?Q0O, 1lN~|r(9Q0KOJ
13

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6.3

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2M8%
[1℄ Eddington, A.S., 1930: The Internal Constitution of the Stars.
Cambridge: Univ. Press Cambridge[2℄ Cowling, T. G., 1934: The Stability of Gaseous Stars. M on. N ot.
Roy . Astron. So ., Vol. 94, p. 768[3℄ Hitotuyanagi, Zyuiti, 1935: Bemerkungen uber ein Sternmodell mit
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and Pulsational Stability of Variable Stars. I. Os illations of LongPeriod Variables. Astrophys. J ., Vol. 499, p. 355[12℄ Xiong, D. R., Deng, L., 2007: Non-adiabati Os illations of Red
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[13℄ Takeuti, M., Aikawa, T., 1981: Resonan e Phenomenon in Classi al
Cepheids. S i. Rep. T o^hoku U niv., Ser. VIII, Vol. 2, p. 106

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