ブラックホール天体のX線エネルギースペクトル中に広がった鉄輝線のように見える構造の解釈について
全文
(2)
(3) ! "#$%& ' ( ). *+,. -.
(4) . .. /+0. 1. 2. 252ῌ5210 3ῌ1ῌ1. e-mail: [email protected].
(5) X . !". #$ %&'()*+,-./01234.56789 :;<=> ?@A BCDEFG>H I JK LMNOPQR.STUV W BC.XYG>7Z [\']^_`1a7bc.deG>H \7 W :;A89BC.fghiAjk'l >mnop I q MCG-6-30-15 cr.stuvwV W xy.z{| }~r'XYG>7Abc.BV7 ' W`.G>H 7 bc 'G> _`>:;A D789 EFP "`A6H. DG> "#$Z`. 7689 EF ¡Y_`16A6H :DEFGHIb <$-./. 1. 3 4 5 . IDEFGHI%`/,+ah`/2)8. !"#
(6) $%&!'".
(7) !3DEFGHI%:RS:^_. ()*+,-./0,123 4/,0+. "# X WXWX3*6.YZ!:e+df. 56.-7+8 9:;<:="# >. [Z"%`/d+db# X K . ?@AB?@C:DEFGHIJ: X. b5<# # &' j3,6.!S. KLMG3NOPQ3*6.R<S. (5)*%`/8 [Z43# q%39. TU-!VK"WXYZ..# [Z". 2010 + 3 93,"'5-d# 3 9. DEFGHI:\]:^_%`/# ,+a. , 6 93[ZZ./ 0,1"W. Nbc3-!0,"`/:%b5de+df. X5-dI-# ¡:¢().. [:*+5LMG ghi5j". /8 w£-35/dh-Z5"#
(8) $%b. klmI I n?@ MCG-6-30-15 %`o# p`. Y3[Z:¤,b¥6!W2d0:)*. qdr sJ3*/t"6!VK:u" # D. :3¦§¨,4©ª«q/,,h3# ¬#. EFGHI:\]:^_,-.. &!'"# MCG-6-30-15 :zI®3¯¢°. 1). vw!8. %. 7!# qx<sJ:LMG3O-.O. -.5!±Q:²(uq/3)ῌ5)8 &!'b# ¬. 3t"6!VKyz!.bw# [:"{|. :³E´II% 1ῌ40 keV ,+tµ¶. }"~~DEFGHI%YZ. ·I6¸3¹!/LMG7ºa8q/#. /h:*ohb/d3#!w# MCG-6-30-15. »!5LMGyz9¼q/8 &!':y. : 103 ½. :7. 445.
(9) Sgr A῏
(10) ῎῎῎῎῎῎῎῎῎῎῎῎῎῎῎῎῎῎῎῎῎῎῎῎῎῎῎. 1. EXOSAT ²¢6) i¡l y³7{ ²¢10) i´l IJ)*+,-(&¢µ'(£ X-1 mno( pq,r ¥Z¦ §+r]¨©L¤ w¶·=0EKW¸j+¦¹' ºrpq,r%T »¼.
(11)
(12) . 1980 u/0%T 1984 v=wx04. . y 7z{ |(}+b EXOSAT ]. . !"#$ %& '()*+,. 4~4 ]4R imn. -(.#
(13) /0123456 789. o(% DE/Eῌ20l mno( . :;4 <=>. ! "4 (DE/Eῌ7) L. ?@A34 BCD EF
(14) . HL0/ 4. GHIJKALM N O.
(15) @ (6.4 keV) # (6.7. EPQ% RS ?%TU. keV) # (7.0 keV) $%Z. V. )*+,-(.#
(16) /0W XF4. .
(17) YZ 78. 4L
(18) X . :;IJ A34 [0\ ]>. X
(19) E%8U.
(20) 04)*+,-(^_`ab*.
(21) B/0)8 fz. . 1 i¡l EXOSAT )*+,-( & ¢ ' ( £ X-1 m n o ( p q , r L ¤. c(d(e%Z. 6) ¥Z¦ §+r ]¨©L¤. 2. ῐ῎῏῍ῌ. 0/ T T. X f 1962 gh K . ª«¬%)
(22) . i. jk 6.4῍7.0 keVl #mn. 8 ®mno(@/012. o(pq,rst J4. 34¯ * 6.2 keV ] °±. 446.
(23) . ½,. 2010 7 ½.
(24) ῍῍῍῍῍῍῍῍῍῍῍῍῍῍῍῍῍῍῍῍῍῍῍῍῍῍῍ Sgr A῎
(25) .
(26)
(27) . X !
(28) z<{s|\O
(29) 9hv. 1987 . %}~131 =
(30). . 20.
(31) K LM*
(32) >
(33) %. cm 9hN ?@A\.
(34) BC. !"
(35) #$% &'()*+. 3.510. %,-#$ .
(36) /. %3105 9h Q ?@D. 01&'()*2 (1.2ῌ37 keV) 345. 1024 cm2 . 6
(37) 789 :
(38) ;<=>?@. 3 .
(39) 3;y LM*&'()* E. ABCD*( E
(40). F!G"
(41) HICJ(K. F 7.1 keV 8 9.3 keV NOP&'. #$8῎ % .
(42) &'(). ()*
(43) X !- G\ .% K 9. . -ELM .U1ha ,. 1.
(44) K LM*NOP&'()*+,:. 0QLM*K#-R . 1
(45) S+ . 7)ῌ12). . /0T X-1. 2.
(46) K LM*%-wx:. -MH =
(47) 1a% 0.34 9 6.4ῌ7.0 keV
(48) , -F!-k.
(49) &'()*HICJ(UV9WXBJ. p ;y%?@D1.51024 cm2 I. YZ[\ ]S
(50) .6\. dJJA-wx:3
(51). :^8 UV8
(52) YZ_`. 9 G X !
(53) K%L" Q. 3HICJ(K#R1a b
(54) 3U. .
(55) -wx1;y dM. c2\89 .
(56) K#%0QF!
(57) . N X !<t
(58) :h1a %. OLM*
(59) ORd 1Uef. <t8
(60) OPC L'8
(61) ,- F. f% 9Ug01&'()*29. ! LM* LC
(62) a^kRv. \34h ij
(63) HICJ(. 315), 16) . & ' ( ) * 2 EXOSAT a ^ k 12.
(64) X !&'()*HICJ(-R,:. keV lmn2UV9WXBJ\. 0 1 L M K # % v
(65) ( 9 Q $ 9 U. h8O 6.2 keV 0QF!5o\. 7)ῌ12), 17) . 2, 3 ]. 10). Rdp
(66) 9h13), 14) MCG-6-30-15 O. @ABCD*(&'. p !-wx1;yhQ1a. qf @ABCD*(&'
(67) X !HICJ(. % LM*LM! ". ()5o\%63. F!/LM*K#. LC%!8J"
(68) 9 b. % 1980 7r8 f-R. "31 LM;y!
(69) Kg. O
(70) 9hN .
(71) stu1
(72) 9: 20 l. 1 KLM
(73) 1aOOPCLMC. O11^9h῎2.
(74) a^k9 R
(75) 01LM*K#v. 3.
(76) v
(77) HICJ(K#% -wx1;y. F!. 9U ij MCG-6-30-15
(78) &'()*HICJ(% KLM(9O Q$\v9U8) . 3 S. ῎1 ij 9%S 1 keV 8 30 keV p9
(79) R
(80) 01&'()*29- T#
(81) U1*V
(82) 9 (8S 1 l
(83) ¡h.¢{9U W r
(84) h\8 XMM-Newton, Chandra . !" X !X£¤ CCD ¢{5
(85) B¥a^k9% &'()*2 10 keV lmn- T#O
(86) 9 (8S 5 lm
(87) ¡hQO¢{\v%Y1 F!Z
(88) 0QHICJ(K#A %
(89) h\8 XMM, Chandra NOP/gQ
(90) 9h ῎2 [¦
(91) \ §]^ % v
(92) _` a&b¨c9!1 h
(93) 9:%1p©
(94) ª*«d¬ vh pg9:
(95) eQ9hN®¯°*±²³!\%´ µf 1
(96) g´
(97) h¶·¸¹
(98) ºi9hQ 8 pg9:%11^g» j 103 ¼. j7½. 447.
(99) Sgr A῎
(100) ῍῍῍῍῍῍῍῍῍῍῍῍῍῍῍῍῍῍῍῍῍῍῍῍῍῍῍. X
(101) !"#$%&'()*+, -. .
(102) /'()*+0. 1234. 56789 (:;<= >?@AB; C7DE18)ῌ20)F GH%I JKLM7N OPQRO0J KSJK TU$3 F W;G XY<. !"#$%V< !"#$Z[. H\ ]^;%_ `ab 2. 3. 448. z} (3ῌ30 keV) +r (0.9 ῌ10 keV) Zw Cyg X-1 l 7 {|lx J"|w17) (Reproduced by permission of the AAS)F s 7wl7F tp ; 2 keV ;¡"?¢lh£ GH%qq ¤;¥<F. c
(103) d _ efd ) dghij k lm3; no9pHF q XY;
(104) r pstH'()*;XuvpHwx 7 qq%y;<pu z{|l$3} ~{q;F {|l$3; <% . z} Zw¢$"#¦§ MCG-6-30-15 l7 x;¨©~{ cªj «¬~{ cj "|w®*¯°8) (Reproduced by permission of the AAS)F ±²p ~{;l7qF >?@AB;C7³w z{|l$3} %´u<F 1 µ¶ ·¸%s ¹º S»3lF ¼½. 2010. 7½.
(105) ῎῎῎῎῎῎῎῎῎῎῎῎῎῎῎῎῎῎῎῎῎῎῎῎῎῎῎ Sgr A῏
(106) .
(107) . +702 * ;
(108) ".
(109) . C9EFGHI8JKEGH. !"#$
(110) % & '. 6Fp+!V)89 +%+ . ()*+,
(111)
(112) ()- *.*./0.
(113) V) &,D*B.
(114) % 1
(115) 2%3%0! "
(116) 45678.
(117) 9 :&tM KE
(118) M
(119) &. 9 DE/Eῌ2:9*. ;<
(120) !.l
(121) KE}I. 2 CCD ; &% <=. ~9"g+
(122) &0 ;
(123) ?M3. >30! &% ? MCG-6-30-15. "C
(124) -.+ EFGHI8JKE.
(125) @AB "C/0 D. =
(126) . M3 . EFGHI8JKEL ?M345 6789*0 .9%+!1). !GH. 4. ῑ῎ῐῌ῏῍ΐῒ. !N+ !?M
(127) / "C. X >?P B@A
(128) B. OPQ R? SC& . C. !=῏3 BGH9. ;
(129) . - DSGHKEHD. XDYZ . ;
(130) [3KE\].
(131) ?MEF,¡3 GHIC. 3 &% B+!"C. + 3%3%J2%3 . M.?,&. ^_`a^b@cd. EFGHI8. ¢ 5,
(132) X >KL@AM6
(133). JKE9 = ;
(134) S e 3 % 10.
(135) ?M3£@AM69 GH. ^_`a^b!f& ."g. M\
(136) ;N%E¤KO . M
(137). TUC.VW2. . . 1) ;S#hO
(138) ij9Y$+. P¥3¦§¨Q& ¤© &%. 3
(139) ;
(140) %k&l3 m. XMM-Newton
(141) B % MCG-6-30-15
(142) /. XMM-Newton h n, B+! MCG-. 0!"C ª ?M3;N. 6-30-15
(143) EFGHI8J2 ;^_`. 3@AM69«.%0!22), 23)¬ (1) . a^boIpHq%d. GH9!RSTU #.. *
(144). 'rEFGH
(145) 's!f 3 ^_`a^b!. EFGHS+ %B. #. f- ?t*()D*9u. !. . S#M6 RS#NM6. = EFGH
(146) 's!f?tv. , MCG-6-. + ?M®Z (2) S#"9. 30-15 +
(147) oIpHqwxy,z,+. VM
(148) /0!" W. . ¯ X
(149) W¯Y M6Z[. {oIpHqN. M-*&. 2), 21). 2 * !?M /0!. °v. . "C;
(150) ./& 01#
(151) KE2. MCG-6-30-15
(152) £ *+*/0!". l,|3
(153) ?0 4!oIp. Y±oIpHqy\
(154) EFGHS?0. Hq
(155) }I~k&l3 . 8]+ .+! '+%+ ²,y\. MCG-6-30-15 * D5,
(156) 6 +h 'oIpHq0. 3 ³ ª
(157) light-bending K E
(158) ´ 9 µ ¶- S#."01#^·+ M. ῏3 ASTRO-H _¸
(159) ¹8H5{5º~ 0.4῍12 keV
(160) W¯ y BC9*2!= X >?P<= DSGH9»;
(161) DD< .l ` 103 ¼. `7½. 449.
(162) Sgr A῍
(163) ῌῌῌῌῌῌῌῌῌῌῌῌῌῌῌῌῌῌῌῌῌῌῌῌῌῌῌ.
(164) .
(165) /
(166) 56.
(167) Matsumoto . w9Y8xH)
(168) !
(169) . . )7%¡8. 23).
(170) ! "
(171) #$. )w9Y8xH . )9>/
(172) - +:f). /
(173) . %&%'()* +,-+. Miniutti / % MCG-. )./
(174) '(0&12% 3. 6-30-15 [\H]7F8GH Wi) light-. 4
(175) ! 56789:;<1+=>. bending IH;P,E) :f) . +
(176) ?@1AB0&. ! &[\H])<¢1£67. >
(177) )CD,E) . 89:;IH>0&1h%2) %. 7F8GH<1IHJ-E. % 0+=>[\H]^. ?@K 0LMN. _M1b?%
(178) 0 . ) O (robust) +#&P=+#QE. n9l1 ¤@0&¥¦. 0 1R) Inoue and Matsumoto. A light-bending IH&. 24). S=,E)TUVW. ! ?@.
(179) / ,-X9Y87Z/ +&+&. §¨& / 7F8GH1X6YG. ?@. )BIHC+0&)D©.
(180) [\H]. ^_),= ` a-&bU.
(181) 1)B. 5E. % cd^_1. ªA+ Minuitti &FG)§¨% light. bU& 9:;?@ef
(182) .. bending IH26)1B / . 1>0&1Jg )h% #%. %H[\H]«0¬1®¯. Wi)3,E
(183) jklGm 3!"n9. I0&1°J%27) #% §¨). lo% p. ,& . !"
(184). q8rs1h)t
(185) =.
(186) X & 1 {|}. H~{H',-±) K
(187) 0&5E. u# 9:;v$& ! ?@. z+%K ! &
(188) )².
(189) 1w9Y8xHy/% z& 1 {|}H. &L³ 678)*%. ~{H'd u()*+M),=. d
(190) /#´)/ &EMe
(191) µ¶. u , - / . light-. 5E ) ªA light bendig. bending IH25) 0 )+
(192). IH
(193) [\H]7F8GH1§¨%. /) w9Y8xH. / [\H]7F8GH1®0. y/%)6781. &1·¸ # ¹%
(194) 28) . ). 0% 678)-. %5 º)CD / NT%MO. =-0&),=
(195) )1.
(196) 7F8GH z» 4, 5 1 light-bending I. 2 &678)3= ! . H0&) #P+ ¹%
(197). (-
(198) 4 . light-bending IHQR¼:¼. ! u()*+M0&),=. - MCG-6-30-15 & !. &43%
(199) ,E)TU &E+. ?@. 0,E
(200) >R)D. ,-
(201) 7F8GH1S. !& 1 {|}H~{H'd>. t=
(202) &P=#QE. 450.
(203) 1¬. ) )). T=½. 2010 U 7 ½.
(204) ῎῎῎῎῎῎῎῎῎῎῎῎῎῎῎῎῎῎῎῎῎῎῎῎῎῎῎ Sgr A῏
(205) . 4. l2a-m 4 RXTE Z[# * ¡ MCG-6-30-15 & 6῍10 keV ¢ 4' ()*£*'4&¤¥$ `a`>k> ¦§ ¨'©
(206) '()* ª«#. X ¢ ¬`'()*£*' 10 keV vw&'()*&®H ¯°?±²¬` $. @ABC)D"!E-43F
(207) GH . 34. I#.J K< LM#. 78NOP012 34 9I2Q >RS
(208) T $ XMM &UVWX. YZ[
(209) H> \2 keV ] ^
(210) Z[_
(211) T $ Chandra, XMM &Z["! MCG-6-30-15 &'()*+ `a`>Qbc&d
(212) >M ef2 78gh"i. $ ji 5. ¢ 'B '#'()* ³´{ 4M#µ78¶ 78{ .C*#4H& ³´{&·W ¸¹t478{&·W¸¹t&¥º$. '()*4k> l,m n78 &01op!>qZ[rs
(213) T MCG-6-30-15 &OP M &k> t&M78N012 34u>$ v wx2 y M78Nz{&|. 5. ῒΐ῏ῐῑ῍ῌ῎ Chandra High Energy Transmitting Grating Spectrometer (HETGS)
(214) CCD CCD . }~ &
(215) Chandra, XMM v;& M78N&S . p')B . '()*.!RS.
(216) H>$ Miller ! M &k> h&M78N. (DE/Eῌ0.5)
(217) !"#$. 478 p')@. % MCG-6-30-15 &'()*+. *op. ,-./ 6.4 keV &012 34 5. >#
(218) l2a-m Chandra, XMM &Z['. 6
(219) 6.7 keV, 7.0 keV 7801. ()*. 2 34. &opBd-
(220) . » 103 ¼. 9:#$ ;<=>-4?& »7½. '(). # 3 4ji x
(221) H 34. I#29)$ #"#. 451.
(222) Sgr A῎
(223) ῍῍῍῍῍῍῍῍῍῍῍῍῍῍῍῍῍῍῍῍῍῍῍῍῍῍῍.
(224) . F ]!^_` RXTE [+. . y,z>WH%4( 4)%VG'. !"#$%&' ()* +,. ("% Chandra HETGS Mg, Si, Fe. -./01!2 34 56. G78CH &I &. 789/04 * (:
(225) ;<=>. ;Fx)' =t Mg He. ? )@A ? )BCDE4/0!. " H "-.# Fe He " H "-.H. #F
(226) FG ;' H(. 78C! (H4!. A! <IJ KL. O¡<#%4/0%VG% 5%<. M
(227) FGN;G%<G'. * ¢G &< 789+,%&". 30). 31). 6. ῒῌ῍῎ῐ῏ῑῌVariable Partial Covering ῐ῏ῑ. #e' =) Fe 78C-£.4&
(228) eHG"#H¤ 789 & 4 ;G#:¥H' / Mg . "
(229) FGOPQ R)S4TU+. 4 $#V4 H "-.H ¦#V. * %V>WXG %. 4§ He "-.H78C-£.
(230). YZ%V[+D\!"#. _G"#H $_G# 789. #; MCG-6-30-15 ]!^_` Chandra,. &k¨! &4('(&w. RXTE
(231) + a b G. "#%0© &4k #F"#. ). 3)ῌ5). cd. ' ]!^_` 4 1ῌ40 keV e)?fg. h i Chandra 4BCQW)fg h . e )' ª [+u; m0©. RXTE 4 10 jke)l. ;)«$!##< =^. m# (n@G< . =G - QW #. % (H5o6p!"#qr. &
(232) x)' =t ¬. sd )'. Hjw/04m®G. =t [+uvt. ¯ (1) °/Hb_±1BC {6.4. !^_ RXTE + 10 keV jw. keV -£.²20 eV| # (AI!2). fgh x 6ῌ10 keV y. +,=)4 H±3. z#(A! 0.5ῌ3 keV {=)4 2ῌ4. {49³²0.6p 5&|' (2) &¢G 7. keV| yz. {}yg~| . 89' (FS ¤ &#'(&4. =^=G - %V@;. % & =)4'(&>W. "# W) { 4|' !"4#. ;' (3) R)S6´7µ!xV. 4 10 jke) (@. ¶' xV4% ·¸ ¶ {&| >. ; yzH}yg. W ;' (4) 78¹DE<. {Wk 3| "#$. +,=)478'. H;)4*%&' ($#;. (4) ; +,# ;)º. (1) %xV ;. 789
(233) 784
(234) _»). (2) Ck/0! 789. «¼! ""%4 MCG-6-30-15 &. & ; (3) Ck 789'. ;)#V (H& {·¸ ¶|. (& ; #F &. #6´&8;)' &¶«. 452. 9½#. 2010 7 ½.
(235) ῍῍῍῍῍῍῍῍῍῍῍῍῍῍῍῍῍῍῍῍῍῍῍῍῍῍῍ Sgr A῎
(236) . cm2, log xn1.6 leVSr56 =t s u"
(237) >Jv0H w"Gm.bxSH. 34 656 GH. 7"Zy"LDB. z{|}:\~ M wO
(238) .A. 6 "Z 1ῌ40 keV " %
(239) ("#$%' "#$ %' ">
(240) 46. mR": :" %pqQ
(241) @ 6. M;aAO ´µ"5¶ %V0 6·; Zf¸6 ¹ ² <
(242) p0 ).78Xp9"v ²<
(243) '2 . 6 !":D? s. u;H @ " º »0 9"v ²<"Gm+N 6. 774 4, 5 0T;? J2 %. q !R")**0 7. "Gm6 R": :"!R") *0; m7
(244) % m rR"#$: :0; .
(245) !"#$%&'("#$%'") *+. , +-./)*012 34 556. 72
(246) 89:0; X <=
(247). m7. 6 %V" Z !2
(248) 89:cV" X <"mel 2pq"KL0 GH. IJ2 c . m Mw :O 6 ("#$%' N 1 "!2. >?@A %
(249) BC !20D2D2"E<. N 2 . F. GH. : CN2/N &'Gm6 %V
(250) . O5 PN. : :" %":. GAQ
(251) @ 6 R>? 4 5
(252) (4) ". ^( .¡w)?L.
(253) G?S G S"PN. m!R"¡wcV¢ !2*. 70 7TU. V2;. IJ2 KL0 %. 389:0 M+NI2. 6. 72
(254) Matsuoka V 0 MWX0O " 8). NN 1 N 2 w. "
(255) £ . !2¤2¥¦LDB +§; m¨. Q
(256) ; YPN Z 34 3 ". .©ª«,¬-5)6 7"Gm. [\5 0 !7]D2^" .
(257) £ +§.
(258) G?_`" M;aAO "bLD. {|}:" %"KL®; >J. B 7
(259) @.cH" de
(260) =. !":.¯; %0. 6 fg de"Z
(261) hi. GADc 6 /. " 3 j" ; k (a) Mg, Si. ¢
(262) £ . .l" <m 3NHn3.7o10. +@" %"KL 35 . 21. 2. *V2. 4 7 ¡w 20,000 0. cm , log xn1.5 leVcpq0 %5 (b) Fe. %V"Zw. " < m _ 3N H n 2.4 o 1023. :pq %JB@°1J2 . 2. cm , log xn3.4 leVSr5 (c) . %"KL 3Z5 T6 2 4 ±Q
(263). m s 3NHn1.6o10. Mv0HGm+N ²<O ³3" 4. 24. 2 103 ¼. 27½. 453.
(264) Sgr A῍
(265) ῌῌῌῌῌῌῌῌῌῌῌῌῌῌῌῌῌῌῌῌῌῌῌῌῌῌῌ. P7. P8. MCG-6-30-15 @AD)^D 7 _ DE+F. WMQRUV\][ \ H IJKLMN+O-8` bUMc* Fµ¶. P9. /e MCG-6-30-15 <=. X !·\ ¸"#\T_& 0123 W+)[ ¹º B HIJKLMN+O-8 >?&5 @A8DE+F.8\G:e. 7 20,000 ª«K¬DE+F.\ fDE+F.\®7 aTg fDE+F.\®7 aT\¯° DE+F.8 67 W>?± ²[ /<=. HI JKLMN+O-`\8&a V ³&5DE+F.867 W<=. ; ´[.
(266) Inoue and Matsumoto24) . !"#$%&' ()*+. ,-./ X !0123
(267) 4&5 678
(268) 9: ; <=. ' >?&5@A$B5 CDE+F.8'GHIJKLMN+O8
(269) :&5 P 8 MQR @AST%UV WP 5 XY 5Z[ \]
(270) @AD)^D 7 _ DE+F._
(271) HIJKLMN+O-`. ; ()*+,-.\v . \8&a
(272) bUMc*F\de @A. ;9$
(273) % X !!. f/g%_5
(274) HIJKLMN. &123 B5/ X !\. +O-'hijk
(275) lm)n-. 4eHIJKLMN+O-8 >?&. O-'eo
(276) DE+F._
(277) pq ;. 5G%@A8DE+F.8\:e. 1 keV / 40 keV rs.t-uv. B5/ 123'$
(278) % 012. wxyz%DE+F.8w_. 3 W{ b [ ; /'12. m)n-O- 9 9{| . 3\e W+)[ ' (1) 0 . '} B5<=. ~\d. opaque % WX !\q&% [ R (2) 0.
(279) T /'
(280) . F ¡K¢
(281) 3e£¤~¥¦f. 3~/
(282) 'P 9 % 454. § 1 ;¨© W{0 123 c »¼. 2010 ½ 7 ¼.
(283) ῌῌῌῌῌῌῌῌῌῌῌῌῌῌῌῌῌῌῌῌῌῌῌῌῌῌῌ Sgr A῍
(284) . (3)
(285) . >!HI!/. a
(286) . @q(L1 ASTRO-H ZI5. . <=>=Q/[\ 3 . !" #$ %. M&28@. X &'()* . 4 Hw=H$ V!1. +( ,-. +( ./01 % 1. VW XY. . rs]A^ _`. 2 $ 3 4 % Broad Line Region. a/bc4/@U/ .1 de. (BLR) 5678
(287) !$1. X Df
(288) E=>g! uFQHh. 9 X :. ij!U/ dkq!/ NASA/GSFC $1. ,/ ;6<=>= ?4. OlB)+(/\ 1 $U@-m. % BLR 5678;6<=>=1@/.
(289) !n[ ST$. A!3), 4). o%/E=>uFQH1 p “easy”. BC DEF !"!EGH56. @-$1qr$ “very easy” $1. IJDEF#%K$%!L. s. M&!K/ EGH5 N'O;6<=. / GSFC $h4%/ “xspec” c%. >=!EGH56IJ(P( %. ;` =¡. 4.5 QRSFTQF8'O )UV 1*. F$#. W X+4%. Y/ 9 ,Z-. $a%/3Hw5aF¤H¥JH#%. 40 eV .[\/]P^DEF. EGH56IJDEF$_G`a( 6`. _G`a1^^b0( %. 5=FH¦J;6<=>=. /c12. h#@ tu!. X Hw5aFuFvwT=. % ¢R£FLd vwuF. §p a. 3QRSFTQF8'O d-EGH545. %! 3&¨ x2$# . 67(2891:;$U e% !. Ye EGH56IJ yh,z yf. f DEF1 g1 QRSFTQF8'. $z©{|4%U/}ª 1 . Ohi<jk=4% lmFn=. X E=>uF. o> ?p/EGH56IJDEF@q. ~«. 1A+%. # A$ rs. very easy !/. #$1 y(¬z RXTE. Chandra £=IE=>D. 7. ῏ ῎ ῍ ῌ. EFKx!/ X Df
(290) d1. rs 1BCEGH56IJD $. ®(E=>. U0¯4%°4%. # MCG-6-30-15 tE E=>uF. $ . v 34%/Hw5aF+BGV;. yv. 6<=>=$HI$UJ/DEFKx!. ´¯(c!@µ. / DEF. . L y[. //] . _±£ $²
(291) ³ $U 1/. 4# r1eC ASTRO-H $,/ MCG-. ,Hw5aFz t{|}M~. 6-30-15 ^LEGH56IJD 3. ^|} 6`5=FNO L$PQ2. f/C y#y1r¶z EGH56IJ. 8R1 rCSTU$#. K/U /·. ¸. / DEF$1[. U@f¶ EGH56IJ@q. j. //] . , !/ VW /. 103 ¼. 7½. @!/%. {. # ¹J¹=Qº»F 455.
(292) Sgr A῏
(293) ῎῎῎῎῎῎῎῎῎῎῎῎῎῎῎῎῎῎῎῎῎῎῎῎῎῎῎.
(294)
(295) %& '()*+,-.!,/ 15
(296) . !" #$. 01233
(297) 4. 06738 9:;<=>'?). @A,!BCDEFGH
(298) IJK 0L M"NO
(299) P0Q 5 RS-TUVW0Q,!,/ 415
(300) . 0123. 06738 "X
(301) YZ[\1. 5])^_
(302) ) H<F;`a506"4b c, X d'ef,gV!h ii5jk
(303) ,lm9n1Oop qrMst u'v,!)wx'y,z0 h ῐ. 15) 16) 17) 18) 19) 20) 21) 22) 23) 24) 25) 26) 27) 28). Titarchuk L, G., 1987, Astrophysics 26, 57 Lightman A. P., White T. R., 1988, ApJ L57 Ebisawa K., et al., 1996, 467, 419 Fabian A. C., et al., 1989, MNRAS 238, 729 Laor, A. 1991, ApJ 376, L90 Kojima Y., 1991, MNRAS 250, 629 Wilms J., et al. 2001, MNRAS 328, L27 Reynolds C. S., 2000, ApJ 533, 811 Matsumoto C., et al., 2003, PASJ 55, 615 Inoue H., Matsumoto C., 2003, PASJ 55, 625 Miniutti G., Fabian A. C., 2004, MNRAS 349, 1435 ῌ Niedz ´wiecki A., Zycki P. T., 2008, MNRAS 386, 759 Niedz ´wiecki A., Miyakawa T., 2010, A&A 509, 22 ῌ Zycki P. T., Ebisawa K., Niedz ´wiecki A., Miyakawa T., 2010, PASJ, submitted 29) Miller L., Turner T. J., Reeves J. N., 2008, A&A 483, 437 30) Reynolds C. S., et al., 2009, MNRAS 397, L21 31) Miller L., Turner T. J., Reeves J. N., 2009, MNRAS 399, L69. ῏ 4{|^,! M}S~op. 6. !). 0 q1 S. ',), >')6. 0. q ,/-h. ῎῍ῑῌ 1) Tanaka Y. et al., 1995, Nature 375, 659 2) Miniutti G. et al., 2007, PASJ 59, S315 3) 2010 ¡IJ¢£ ¤¥S 4) Miyakawa T., Ebisawa K., Inoue H., 2010, PASJ, to be submitted 5) Inoue H., Miyakawa T., Ebisawa K., 2010, PASJ, to be submitted 6) Barr P., et al., 1985, MNRAS 216, 65 7) Inoue H., The 23rd ESLAB Symposium on Two Topics in X-ray Astronomy, Vol. 2, p. 783῍787 ESTEC 8) Matsuoka M., et al., 1990, ApJ 361, 440 9) Pounds K. A., et al., 1990, Nature 344, 132 10) Ebisawa K., 1991, ¡IJ¢£ ¤¥S ISAS Research Note 483 11) Ueda Y., Ebisawa K., Done C., 1993, PASJ 46, 107 12) Ebisawa K., et al., 1994, PASJ 46, 375 13) Tanaka Y., 1991, in “Iron Line Diagnostics in X-Ray Sources,” Lecture Notes in Physics, Vol. 385, p. 98 14) Ebisawa K., 1999, in “Disk Instabilities in Close Binary Systems. 25 Years of the Disk-Instability Model,” Frontiers Science Series No. 26. Universal Academy Press, Inc., p. 203. 456. On the Interpretation of the Seemingly Broad Iron Emission Lines Observed in the X-ray Energy Spectra of Black Hole Objects Ken EBISAWA, MIYAKAWA, and Hajime INOUE Japan Aerospace Exploration Agncy (JAXA)/ Institute of Space and Astronautical Science (ISAS), 3῍1῍1 Yoshinodai, Chuo-ku, Sagamihara, Kanagawa 252῍5210, Japan Abstract : X-ray energy spectra of Active Galactic Nuclei and Galactic black hole binaries commonly indicate a characteristic spectral feature which looks like a gravitationally red-shifted and distorted iron emission line. We review history and background of this problem, and scrutinize some models so far proposed to explain such a spectral feature. We have reanalyzed archival date of the Seyfert I galaxy MCG-6-30-15, which is an archetypal object with such a relativistically distorted iron line feature. Consequently, we propose a new model which can explain the observed spectral variation with minimum numbers of free parameters. Our model rejects presence of the extremely broadened iron emission line which would be expected from very vicinity of an extreme Kerr black hole. We conclude that presence of the relativistically distorted iron emission lines from the very vicinity of the black holes is not observationally established.. £¦§. 2010 ¨ 7 ¦.
(304)
関連したドキュメント
節の構造を取ると主張している。 ( 14b )は T-ing 構文、 ( 14e )は TP 構文である が、 T-en 構文の例はあがっていない。 ( 14a
の後方即ち術者の位置並びにその後方において 周囲より低溶を示した.これは螢光板中の鉛硝
心部 の上 下両端 に見 える 白色の 太線 は管
この節では mKdV 方程式を興味の中心に据えて,mKdV 方程式によって統制されるような平面曲線の連 続朗変形,半離散 mKdV
Then it follows immediately from a suitable version of “Hensel’s Lemma” [cf., e.g., the argument of [4], Lemma 2.1] that S may be obtained, as the notation suggests, as the m A
The main technical result of the paper is the proof of Theorem 3.3, which asserts that the embeddability of certain countable configurations of elements into some model of the
By studying the electromagnetic field associated with a uniformly accelerated charge Boulware 34 made in 1980 an important discovery that he summarized in the following way:
このうち、大型X線検査装置については、コンテナで輸出入される貨物やコンテナ自体を利用した密輸