ᖹᡂ 24 ᖺᗘ ⟃Ἴ኱Ꮫ ィ⟬⛉Ꮫ◊✲ࢭࣥࢱ࣮ ᖺḟሗ࿌᭩II Ᏹᐂ࣭ཎᏊ᰾≀⌮◊✲㒊㛛II-1. Ᏹᐂศ㔝1.

࣓ࣥࣂ࣮ᩍᤵ  ᱵᮧ 㞞அ෸ᩍᤵ ᳃ ṇኵㅮᖌ  

ྜྷᕝ ⪔ྖ

෸ᩍᤵ

ᒸᮏ ᓫ㸦HPCI ᡓ␎ࣉࣟࢢ࣒ࣛ㸧ຓᩍ  ᕝ຾ ᮃ㸦⌮ᩘᏛ⏕ᛂ᥼ࣉࣟࢪ࢙ࢡࢺ㸧◊✲ဨ ㇂ᕝ ⾪㸦⛉◊㈝ᇶ┙㹑㸧⾜᪉ ኱㍜㸦⛉◊㈝ᇶ┙㹑㸧ᕝཱྀ ಇᏹ㸦⛉◊㈝ᇶ┙㸿㸧▼ᒣ ᬛ᫂㸦HPCI ᡓ␎ࣉࣟࢢ࣒ࣛ㸧㛗㇂ᕝ ㈼஧㸦HPCI ᡓ␎ࣉࣟࢢ࣒ࣛ㸧
Alexander Wagner㸦ࢭࣥࢱ࣮㸧Ꮫ⏕2.

኱Ꮫ㝔⏕ 㸯㸰ྡ Ꮫ㢮⏕  㸯ྡᴫせᮏᖺᗘ㸪ᙜࢢ࣮ࣝࣉࢫࢱࢵࣇࡣ㸪 FIRST ࣉࣟࢪ࢙ࢡࢺࢆ᥎ࡋ㐍ࡵࡿ࡜ඹ࡟㸪FIRST,
T2K-Tsukuba ࢆ⏝࠸࡚㸪Ᏹᐂㄽⓗ㖟Ἑᙧᡂࢩ࣑࣮ࣗࣞࢩࣙࣥ㸪⢏Ꮚἲ㍽ᑕὶయ࡟ࡼࡿᏱᐂ
෌㟁㞳ࢩ࣑࣮ࣗࣞࢩࣙࣥ㸪࣓ࢵࢩࣗὶయ⏝㧗㏿㍽ᑕ㍺㏦ィ⟬㸪኱㉁㔞ࣈࣛࢵࢡ࣮࣍ࣝከయ
⣔࡟࠾ࡅࡿࣈࣛࢵࢡ࣮࣍ࣝࡢྜయᡂ㛗㸪ࢲ࣮ࢡ࣐ࢱࣁ࣮ࣟࡢෆ㒊ᵓ㐀㸸ࢥ࢔࢝ࢫࣉၥ㢟㸪࢔ࣥࢻ࣓ࣟࢲࡢᾦ࡜ࡉࡊࡵࡁ㸪㖟Ἑ⣔୰ᚰ㡿ᇦࡢ≉␗࡞≀⌮⎔ቃࡀศᏊ㞼ᙧᡂ࡟୚࠼ࡿᙳ
㡪㸪6 ḟඖ Vlasov ᪉⛬ᘧ࡟ࡼࡿ⮬ᕫ㔜ຊ⣔ᩘ್ࢩ࣑࣮ࣗࣞࢩࣙࣥࡢ◊✲ࢆ⾜ࡗࡓࠋࡉࡽ࡟㸪
AVX ࿨௧∧ Phantom-GRAPE ࡢ㛤Ⓨ㸪HA-PACS ࡟ྥࡅࡓ࢔ࣉࣜࢣ࣮ࢩࣙࣥࡢ㛤Ⓨ㸪ࠕிࠖࢆ⏝࠸ࡓ㖟Ἑᙧᡂࢩ࣑࣮ࣗࣞࢩࣙࣥࢆ⾜ࡗࡓࠋࡲࡓ㸪Ᏹᐂ࣭⏕࿨࣭≀ᛶ࣭ཎᏊ᰾ศ㔝㐃ᦠ࡛ᫍ㛫✵㛫࡟࠾ࡅࡿගㄏ㉳ L ᆺ࢔࣑ࣀ㓟㐣๫㸪⣔እᝨᫍ࡟࠾ࡅࡿගྜᡂ࢔ࣥࢸࢼᶵᵓࡢ⌮ㄽⓗ◊✲ࢆ⾜ࡗࡓࠋࡲࡓ㸪ࣉࣞᡓ␎࢖ࢽࢩ࢔ࢸ࢕ࣈࠕ࢔ࢡࢭ࣮ࣛࣞࢱ࡟ࡼࡿ㖟Ἑ㍽ᑕὶయຊᏛࡢᖥ㛤ࡅࠖ㸦௦⾲⪅ ᳃ṇኵ㸧ࡢ⥅⥆ࡀ᥇ᢥࡉࢀ㸪㍽ᑕὶయຊᏛᐇ⌧ࡢࡓࡵࡢ₇⟬ຍ㏿
ჾࢆᦚ㍕ࡋࡓ୪ิィ⟬ᶵࢩࢫࢸ࣒ᵓ⠏ࢆ㛤ጞࡋ㸪ࣉࣟࢺࢱ࢖ࣉࡢไసࢆ⾜ࡗࡓࠋ
3.

◊✲ᡂᯝ

࠙㸯ࠚ୍⯡┦ᑐㄽⓗ N యィ⟬࡟ࡼࡿᕧ኱ࣈࣛࢵࢡ࣮࣍ࣝྜయ㐣⛬ᕧ኱ࣈࣛࢵࢡ࣮࣍ࣝࡣ㖟Ἑ୰ᚰ࡟ほࡉࢀ㸪ࣈࣛࢵࢡ࣮࣍ࣝ㉁㔞ࡣ㖟Ἑࣂࣝࢪ㉁㔞ࡢ⣙ 1/1000 ࡟࡞ࡗ࡚࠸ࡿ࡜࠸࠺“ࣈࣛࢵࢡ࣮̺࣍ࣝࣂࣝࢪ㉁㔞㛵ಀ”ࡀぢฟࡉ40ᖹᡂ 24 ᖺᗘ ⟃Ἴ኱Ꮫ ィ⟬⛉Ꮫ◊✲ࢭࣥࢱ࣮ ᖺḟሗ࿌᭩ࢀ࡚࠸ࡿ㸦Kormendy & Richstone 1995; Magorrian et al. 1998; Merrifield et al.
2000; Merritt & Ferrarese 2001, Marconi & Hunt 2003㸧ࠋࡇࢀࡣ㸪ᕧ኱ࣈࣛࢵࢡ
࣮࣍ࣝᙧᡂࡀ㸪㖟Ἑࣂࣝࢪᙧᡂྐ࡜ᐦ᥋࡟㛵ಀࡋ㸪ࣈࣛࢵࢡ࣮࣍ࣝ㉁㔞ࢆỴࡵࡿ㝵ᒙⓗኳయᙧᡂㄽ࡟
ᬑ㐢ⓗ࡞≀⌮࣓࢝ࢽࢬ࣒ࡀᏑᅾࡋࡓࡇ࡜ࢆ♧၀ࡍࡿࠋᏱᐂࡢ㝵ᚑ࠼ࡤ㸪኱ࡁ࡞㖟Ἑࡣᑠ㖟Ἑࡢ㞟ྜయ࡜ࡋ࡚⏕ࡲࢀࡿࡇ࡜࡟࡞ࡾ㸪኱ࡁ࡞㖟Ἑ࡟ࡣከᩘࡢᕧ኱ࣈࣛࢵࢡ࣮࣍ࣝࡀᏑᅾࡍࡿࡇ࡜࡟࡞ࡿࠋࡇࢀࡣ㸪㖟Ἑࡢ୰ᚰ࡟ࣈࣛ
ࢵࢡ࣮̺࣍ࣝࣂࣝࢪ㉁㔞㛵ಀࢆ‶ࡓࡍᕧ኱ࣈࣛࢵࢡ࣮࣍ࣝࡀ୍ࡘ࠶ࡿ࡜࠸࠺ほ஦ᐇࢆㄝ࡛᫂ࡁ࡞࠸ࠋྍ⬟ᛶࡢ୍ࡘࡣ㸪㖟Ἑࡀྜయࡋࡓ㝿࡟㸪ࣈࣛࢵࢡ࣮࣍ࣝࡶ
඲࡚ྜయࡋ࡚㸪㖟Ἑ୰ᚰ࡟ⴠࡕࡿ࡜࠸࠺ࡶࡢ࡛࠶ࡿࠋࡋ࠿ࡋ㸪ࡇࢀࡲ࡛ᕧ኱ࣈࣛ
ࢵࢡ࣮࣍ࣝࡢྜయࡣᴟࡵ࡚㞴ࡋ࠸࡜ࡉࢀ࡚ࡁࡓࠋᡃࠎࡣ㸪ࣈࣛࢵࢡ࣮࣍ࣝࢆᣢࡘ
㖟Ἑࡀྜయࡋࡓᚋ㸪ࣈࣛࢵࢡ࣮࣍ࣝྜయࡀ㉳ࡇࡿ࠿࡜࠸࠺ၥ㢟ࢆ㸪୍⯡┦ᑐㄽຠ୍⯡┦ᑐㄽⓗ䠪యィ⟬䛻䜘䜛䝤䝷䝑䜽䝩䞊䝹ྜయ᮲௳䛸ほ 䛸䛾ẚ㍑
䝅䝭䝳䝺䞊䝅䝵䞁䛻䜘䛳䛶ᚓ䜙䜜䛯䝤䝷䝑䜽䝩䞊䝹ྜయ᮲௳z=7 䝷䜲䝬䞁䜶䝭䝑䝍䞊䛾ගᗘ㛵ᩘ⥺䛻௜䛡䜙䜜䛯ᩘ್䛿௬ᐃ䛧䛯㉁㔞䠉ගᗘẚ⦪䛾Ἴ⥺䜘䜚ᕥഃ䛷ྜయ䛜ྍ⬟Ouchi et al. 2009

Tanikawa & Umemura 2012㧗⢭ᗘ N యィ⟬࡟ࡼࡾㄪ࡭ࡓࠋ㖟Ἑࣂࣝࢪࡢ୰࡟ 10 ಶࡢᕧ኱ࣈࣛࢵࢡ
ᯝࢆධࢀࡓ㧗
࣮࣍ࣝࢆ⨨࠸࡚ィ⟬ࡋࡓ⤖ᯝ㸪㖟Ἑ୰ࡢᫍᐦᗘࡀ㧗࠸ሙྜ࡟ࡣ㸪ᫍ࡟ࡼࡿຊᏛⓗᦶ᧿ࡀ᭷ຠ࡟ാࡁ㸪ࣈࣛࢵࢡ࣮࣍ࣝࡣ㖟Ἑ୰ᚰ࡟ⴠࡕࡿࡇ࡜࡛ከ㔜ᩓ஘ࢆ⧞ࡾ㏉ࡋ㸪㐃ࣈࣛࢵࢡ࣮࣍ࣝࡀ⏕ࡲࢀ㸪㐃ࣈࣛࢵࢡ࣮࣍ࣝࡣ௚ࡢࣈࣛࢵࢡ࣮࣍ࣝ࡜ࡢᩓ
஘ࡢ⤖ᯝ㸪㔜ຊἼࢆᨺฟࡋ࡚ྜయࡍࡿࡇ࡜ࡀศ࠿ࡗࡓࠋࡑࡋ࡚㸪ࣈࣛࢵࢡ࣮࣍ࣝ
ྜయࡀ࡝ࡢࡼ࠺࡞㖟Ἑ࡛㉳ࡇࡾ࠺ࡿ࠿࡜࠸࠺ࡇ࡜ࢆゎᯒࡋࡓ⤖ᯝ㸪ࡍࡤࡿᮃ㐲㙾࡛ぢ࠼࡚࠸ࡿ㉥᪉೫⛣ z=7 ࡢࣛ࢖࣐ࣥ࢔ࣝࣇ࢓࣭࢚࣑ࢵࢱ࣮࡛㸪ࣈࣛࢵࢡ࣮࣍ࣝ

41

ᖹᡂ 24 ᖺᗘ ⟃Ἴ኱Ꮫ ィ⟬⛉Ꮫ◊✲ࢭࣥࢱ࣮ ᖺḟሗ࿌᭩ྜయ㐣⛬ࡀ㉳ࡇࡗ࡚࠸ࡿྍ⬟ᛶࢆ♧ࡋࡓ㸦ୗᅗ㸧ࠋ࠙㸰ࠚ ➨୍ୡ௦ኳయࡢ㍽ᑕὶయィ⟬Ᏹᐂ࡛᭱ึ࡟⏕ࡲࢀࡓኳయ(➨୍ୡ௦ኳయ)ࡣ㸪ᚑ᮶ࡢィ⟬࡛ࡣ |106M~ࡢࢲ࣮ࢡ࣐ࢱ࣮ࣁ࣮ࣟ࡟ |105M~⛬ᗘࡢࣂࣜ࢜ࣥ
࢞ࢫࡀ⵳✚ࡉࢀ࡚ᙧᡂࡉࢀࡿ࡜ࡉࢀ࡚ࡁ
ࡓࠋࡋ࠿ࡋ࡞ࡀࡽ㸪ᚑ᮶ࡢ◊✲࡛ࡣ㸪ࢲ࣮ࢡ࣐ࢱ࣮ࡢᑠࢫࢣ࣮࡛ࣝࡢ᣺ࡿ⯙࠸㸪≉࡟ࢲ࣮ࢡ࣐ࢱ࣮࣭࢝ࢫࣉࡢᡂ㛗࡟ࡘ࠸࡚ࡣ࠶ࡲࡾὀ┠ࡉࢀ࡚ࡇ࡞࠿ࡗࡓࠋࡑࡇ
࡛㸪ᡃࠎࡣィ⟬㡿ᇦࡢ඲యࢆྍ⬟࡞㝈ࡾ㧗ゎീᗘ࡟ࡋࡓᩘ್ィ⟬࡛㸪ࢲ࣮ࢡ࣐ࢱ
࣮࣭࢝ࢫࣉࡢᡂ㛗ࢆศゎ࡛ࡁࡿࡼ࠺࡟ࡋ㸪➨୍ୡ௦ኳయࡢᙧᡂ࡜㐍໬ࢆㄪ࡭ࡓࠋ
ࡇࡢィ⟬࡛ࡣ㸪ࢲ࣮ࢡ࣐ࢱ࣮࡜ὶయ⢏Ꮚࢆࡑࢀࡒࢀ⣙ 1 ൨య(5123 య)౑࠸㸪ィ⟬㡿ᇦࡢ඲య࡟ࢃࡓࡗ࡚ࣂࣜ࢜ࣥ࡜ࢲ࣮ࢡ࣐ࢱ࣮㉁㔞ゎീᗘ࡜ࡋ࡚ࡑࢀࡒࢀ
0.046M~࡜ 0.22 M~ ࢆᐇ⌧ࡋࡓ㸦ྑᅗ㸧ࠋࡑࡢ⤖ᯝ㸪➨୍ୡ௦ኳయࡢ㉁㔞ࡣᚑ᮶ࡢィ⟬࡛ồࡵࡽࢀ࡚࠸ࡓ㉁㔞ࡼࡾ 2 ᱆㏆ࡃᑠࡉࡃ࡞ࡿ㸦|103M~⛬ᗘ㸧ࡇ࡜ࡀࢃ࠿
ࡗࡓࠋࡇࡢ⤖ᯝࡢ୍㒊ࡣ㸪᪤࡟≉ู᥎㐍◊✲࡛ᚓࡽࢀ࡚࠸ࡓࡶࡢ࡛࠶ࡿࡀ㸪ࡑࡢᚋࡢゎᯒ࡛㸪ࢲ࣮ࢡ࣐ࢱ࣮࣭࢝ࢫࣉࡢ㔜ຊ࣏ࢸࣥࢩࣕࣝࡀ㸪ࣅࣜ࢔ࣝᗘࢆୖ᪼ࡉࡏ㸪ࡑࡢ⤖ᯝỈ⣲ศᏊ෭༷ࡢ⇕ⓗ୙Ᏻᐃࢆᘬࡁ㉳ࡇࡍࡇ࡜࡛ᑠ㉁㔞ࡢኳయᙧᡂ
ࡀྍ⬟࡟࡞ࡿࡇ࡜ࢆ᫂ࡽ࠿࡟ࡋࡓ㸦Umemura et al. 2012㸧ࠋ࠙㸱ࠚ ཎጞ㖟Ἑᙧᡂ࡜Ᏹᐂ෌㟁㞳Ᏹᐂࡣ㉥᪉೫⛣ z=1000 ⛬ᗘ୍࡛ᗘ୰ᛶ໬ࡋ㸪ࡑࡢᚋᙧᡂࡉࢀࡓኳయ࠿ࡽࡢ㍽ᑕ࡟ࡼࡗ࡚
෌ࡧ㟁㞳ࡋࡓ࡜⪃࠼ࡽࢀ࡚࠸ࡿࠋࢡ࢚࣮ࢧ࣮྾཰⥺⣔ࢆ฼⏝ࡋࡓほ(e.g., Fan et al. 2006)࡛ࡣ㸪z=6 ⛬ᗘ࡛ࡣࡍ࡛࡟Ᏹᐂࡣ㧗ᗘ࡟㟁㞳ࡉࢀ࡚࠸ࡿ஦ࡀ♧ࡉࢀ࡚࠸ࡿࡀ㸪ࡇࡢᏱᐂ෌㟁㞳㐣⛬ࡀ࠸ࡘጞࡲࡾ㸪࡝ࡢࡼ࠺࡟㐍ࢇࡔ࠿ࡣᮍࡔ᫂ࡽ࠿࡛ࡣ࡞࠸ࠋᏱᐂ෌㟁㞳ྐࢆゎࡁ᫂࠿ࡍ࡟ࡣ㸪㖟Ἑ㛫✵㛫࡬ࡢ㟁㞳ගᏊ౪⤥※࡛࠶ࡿኳయࡢᙧᡂྐ࡜ࡑࢀ࡟క࠺㟁㞳㡿ᇦࡢ㐍໬㐣⛬ࢆྠ᫬࡟ィ⟬ࡍࡿᚲせࡀ࠶ࡿࡀ㸪ࡇࡢኳయᙧᡂྐ⮬య࡟㍽ᑕᛶࣇ࢕࣮ࢻࣂࢵࢡࡀᙳ
㡪ࢆཬࡰࡍⅭ㸪㍽ᑕὶయィ⟬ࡀᚲせ࡜࡞ࡿࠋࡇࡢࡼ࠺࡞ィ⟬࡛ࡣ㸪ከࡃࡢᨺᑕ※ࢆྲྀࡾᢅ࠺ᚲせࡀ࠶ࡿⅭ㸪㠀ᖖ࡟⭾኱࡞ィ⟬ࢥࢫࢺࡀせồࡉࢀࡿࠋࡑࡇ࡛㸪ᡃࠎࡣ⊂⮬࡟㛤Ⓨࡋࡓࢶ࣮ࣜᵓ㐀ࢆ⏝࠸࡚㧗㏿࡟㍽ᑕ㍺㏦ィ⟬ࢆ⾜࠼ࡿࢫ࣮࣒࢟ START (SPH with Tree-based Accelerated Radiative Transfer) (Hasegawa &Umemura 2010)ࢆᏱᐂㄽⓗ㍽ᑕὶయィ⟬࡟ᑐᛂ࡛ࡁࡿࡼ࠺࡟ᣑᙇࡋ㸪ࡇࢀࢆ⏝࠸࡚Ᏹᐂ෌

42

ᖹᡂ 24 ᖺᗘ ⟃Ἴ኱Ꮫ ィ⟬⛉Ꮫ◊✲ࢭࣥࢱ࣮ ᖺḟሗ࿌᭩㟁㞳ࢩ࣑࣮ࣗࣞࢩࣙࣥࢆ⾜ࡗࡓࠋࡑࡢ⤖ᯝ㸪Ᏹᐂࡢᫍᙧᡂྐࡣ୺࡟ගຍ⇕ຠᯝ࡟ࡼࡗ࡚ⴭ
ࡋࡃ㜼ᐖࡉࢀࡿ஦ࢆ♧ࡋࡓ(Hasegawa & Semelin 2013)ࠋࡲࡓ㸪෌㟁㞳㐣⛬࡟࡜ࡗ࡚㔜せ࡞㘽࡜࡞ࡿ㟁㞳ගᏊࡢ㖟Ἑ࠿ࡽࡢ⬺ฟ๭ྜࡣ㸪⣸እ⥺ࡢࣇ࢕࣮ࢻࣂࢵࢡ࡛㧗ᐦᗘ㡿ᇦࡀ࡞ࡽࡉࢀࡿ஦࡟ࡼࡗ࡚ୖ᪼ࡍࡿ஦ࡶศ࠿ࡗࡓ(Umemura et al. 2012)ࠋ
ࡲࡓ㸪௒ᖺᗘࡣிࡢࡼ࠺࡞኱つᶍ୪ิィ⟬ᶵ࡛ຠ⋡ࡀฟࡏࡿࡼ࠺ START ࡢ࢔ࣝࢦࣜࢬ࣒
ࡢᨵၿࡶ⾜ࡗࡓࠋࡑࡢ⤖ᯝ㸪ᩘ 1000 ୪ิ௨ୖ࡛ࡢィ⟬࡛࠶ࡗ࡚ࡶ㠀ᖖ࡟ࡼ࠸ࢫࢣ࣮ࣛࣅࣜ
ࢸ࢕ࢆᐇ⌧ࡍࡿ஦ࢆྍ⬟࡟ࡋ㸪₇⟬ᩘ⮬యࡶ࠾ࡼࡑ༙ศ࡟ࡍࡿ஦࡟ᡂຌࡋࡓ(START2:
Hasegawa in prep.)ࠋ
࠙㸲ࠚ ࠕிࠖࢆ⏝࠸ࡓࢲ࣮ࢡ࣐ࢱ࣮ࢩ࣑࣮ࣗࣞࢩࣙࣥ
⌮໬Ꮫ◊✲ᡤࡢிࢥࣥࣆ࣮ࣗࢱୖ࡛㸪㔜ຊከయࢩ࣑࣮ࣗࣞࢩࣙࣥ⏝ࢥ࣮ࢻ"GreeM" ࢆࢳ࣮ࣗࢽࣥࢢࡋࡓࠋᡃࠎࡣ㸪ᩘ୓ࡸᩘ༑୓୪ิ࡛ࡶࢫࢣ࣮ࣝࡍࡿࡼ࠺࡟௨ୗࡢ᭱㐺໬ࢆ⾜ࡗࡓࠋ1) ኱つᶍ࡞඲ᑐ㏻ಙࡢ㝵ᒙ໬ࠋࡲࡎ඲ࣀ࣮ࢻࢆ࠸ࡃࡘ࠿ࡢࢢ࣮ࣝࣉ࡟ศ๭ࡍࡿࠋࡇࡢ᫬㸪✵㛫ⓗ࡟㏆࠸㡿ᇦࢆᢸᙜࡍࡿࣀ࣮ࢻࡀྠࡌࢢ࣮ࣝࣉ࡟࡞ࡿࡼ࠺࡟ࡍࡿࠋࡑࡋ࡚ࢢ࣮ࣝࣉෆ
࡛ࡢ඲ᑐ㏻ಙࢆ⾜ࡗ࡚࠿ࡽ㸪ࢢ࣮ࣝࣉ㛫࡛㏻ಙࡍࡿ࡜࠸࠺ࡼ࠺࡟2 ẁ㝵࡟ศࡅ࡚㏻ಙࢆ⾜࠺ࡇ࡜࡟ࡼࡗ࡚඲ᑐ㏻ಙࡢᐇ⾜᫬㛫ࢆᢚไࡋࡓࠋ
2) 㡿ᇦᙧ≧ࢆ㐣ཤࡢᩘࢫࢸࢵࣉ࡟Ώࡗ࡚ᖹᆒ໬ࡍࡿࡇ࡜࡟ࡼࡾ㸪ࢧࣥࣉࣜࣥࢢ࡟ࡼࡿࢫࢸ
ࢵࣉ㛫ࡢᙧ≧ࡢࡤࡽࡘࡁࢆᢚ࠼㸪⢏Ꮚ෌㓄ศࡢ㏻ಙࢥࢫࢺࡢᢚไࠋ
3)

MPI+OpenMP ࡟ࡼࡿࣁ࢖ࣈࣜࢵࢻ୪ิ໬
ࡇ࠺ࡋ࡚ிࢥࣥࣆ࣮ࣗࢱୖ࡛࡯ࡰ᏶⎍࡞ࢫࢣ࣮ࣛࣅࣜࢸ࢕ࢆᐇ⌧ࡋࡓࠋࡉࡽ࡟2඙ࢲ࣮ࢡ࣐ࢱ࣮⢏Ꮚࡢ㔜ຊ㐍໬ࢩ࣑࣮ࣗࣞࢩࣙࣥࢆ㸪ிࢥࣥࣆ࣮ࣗࢱࡢ࡯ࡰ඲ࢩࢫࢸ࣒ࢆ⏝࠸࡚㸪
5.67 ࣌ࢱࣇࣟࢵࣉࢫࡢᐇຠᛶ⬟(ᐇ⾜ຠ⋡55%) ࡛ᐇ⌧ࡋࡓࠋࡇࢀࡽࡢᡂᯝࡀㄆࡵࡽࢀ㸪ࣁ࢖࣭ࣃࣇ࢛࣮࣐ࣥࢫ࣭ࢥࣥࣆ࣮ࣗࢸ࢕ࣥࢢ࡟㛵ࡍࡿᅜ㝿఍㆟SC12㸦2012 ᖺ11᭶㸪⡿ᅜ࣭ࢯࣝࢺࣞ࢖ࢡࢩࢸ࢕㛤ദ㸧࡟࠾࠸࡚㸪ࢦ࣮ࢻ࣭ࣥ࣋ࣝ㈹ࢆ༢⊂ཷ㈹ࡋࡓࠋࢦ࣮ࢻ࣭ࣥ࣋ࣝ㈹ࣇ࢓࢖ࢼࣜࢫࢺ࡟ࡣ㸪ࣆ࣮ࢡᛶ⬟ࡀ20 ࣌ࢱࣇࣟࢵࣉࢫ(ࠕிࠖࡢ⣙2ಸ) ࡢࠕࢭࢥ࢖࢔ࠖ㸦( ⡿ᅜ࣭࣮ࣟࣞࣥࢫ࣭ࣜࣂࣔ࢔ᅜ❧◊✲ᡤ㸧ࢆ⏝࠸࡚㸪ྠᵝࡢࢲ࣮ࢡ࣐ࢱ࣮ࢩ࣑࣮ࣗࣞࢩࣙࣥ
࡛14 ࣌ࢱࣇࣟࢵࣉࢫࢆ㐩ᡂࡋࡓ⡿ᅜࡢࢢ࣮ࣝࣉࡀ࠶ࡗࡓࠋ࡜ࡇࢁࡀᡃࠎࡢࢥ࣮ࢻࡀᐇ㝿ࡢィ⟬㏿ᗘ࡛ୖᅇࡾ㸪1 ⢏Ꮚ࠶ࡓࡾ2.4 ಸࡢ㏿ࡉ࡛ࢩ࣑࣮ࣗࣞࢩࣙࣥࢆࡍࡿࡇ࡜ࡀྍ⬟࡛࠶ࡗࡓ(ྠࡌィ⟬ᶵࢆ⏝࠸ࡓሙྜࡣ5 ಸ㏆ࡃ㏿࠸)ࠋࡇ࠺࠸ࡗࡓⅬࡀホ౯ࡉࢀ㸪ࢦ࣮ࢻ࣭ࣥ࣋ࣝ㈹ࡢཷ㈹࡟ࡘ࡞ࡀࡗࡓࡼ࠺࡛࠶ࡿࠋ
࠙㸳ࠚ άື㖟Ἑ᰾ࢪ࢙ࢵࢺࡢࣉࣛࢬ࣐⤌ᡂࡢ◊✲άື㖟Ἑ᰾࠿ࡽᄇฟࡍࡿ┦ᑐㄽⓗࢪ࢙ࢵࢺࡢࣉࣛࢬ࣐⤌ᡂࡀ㸪㟁Ꮚ࣭㝧Ꮚ࡞ࡢ࠿㸪 ࡑࢀ43

ᖹᡂ 24 ᖺᗘ ⟃Ἴ኱Ꮫ ィ⟬⛉Ꮫ◊✲ࢭࣥࢱ࣮ ᖺḟሗ࿌᭩࡜ࡶ㟁Ꮚ࣭㝧㟁Ꮚ࡛࠶ࡿ࠿࡜࠸࠺᰿ᮏⓗ࡞ၥ㢟ࡣᮍࡔ᫂ࡽ࠿࡟࡞ࡗ࡚࠸࡞࠸ࠋ ࡇࢀࡣ㸪┦ᑐㄽⓗࢪ࢙ࢵࢺࡢᙧᡂ࣓࢝ࢽࢬ࣒ࡸᏱᐂ⥺ࡢ㉳※࡜ࡶ㛵㐃ࡍࡿᏱᐂ≀⌮Ꮫ࡟࠾࠸࡚᭱㔜せࢸ࣮࣐ࡢ㸯ࡘ࡛࠶ࡿࠋࡇࢀࡲ࡛㸪ࣂࣝࢡࢥࣥࣉࢺࣥ ࡜࿧ࡤࢀࡿ㸰ḟⓗᨺᑕࡢ᭷↓㸪ࢩࣥࢡࣟࢺࣟࣥ⮬ᕫ྾཰ࡸ෇೫Ἴᡂศ࠿ࡽ㸪 ࣈ࣮ࣞࢨ࣮ࢪ࢙ࢵࢺ୰ࡢࣉࣛࢬ࣐⤌ᡂ࡟ࡘ࠸࡚ࡢ㆟ㄽࡀࡉࢀ࡚ࡁࡓࠋ ࡋ࠿ࡋ㸪ࣉࣛࢬ࣐⤌ᡂ࡜ᐦ᥋࡟㛵ಀࡍࡿ┿ࡢࢪ࢙ࢵࢺࣃ࣮࣡ࢆホ౯ࡍࡿࡇ࡜ࡣ ᅔ㞴࡛࠶ࡾ㸪ᚑ᮶ࡢᡭἲ࡛ࡣᨺᑕගᗘ࠿ࡽ㢮᥎ࡍࡿ࡯࠿࡞࠿ࡗࡓࠋ ࡇࡢၥ㢟ࢆゎỴࡍࡿࡓࡵ࡟㸪ᡃࠎࡣ㸪ࢪ࢙ࢵࢺ࢚ࢿࣝࢠ࣮ࡢ㈓ⶶᗜ࡛࠶ࡿ ⭾ᙇࢥࢡ࣮ࣥຊᏛ࡟ὀ┠ࡋ㸪┿ࡢࢪ࢙ࢵࢺࣃ࣮࣡࡜ᖺ㱋ࢆホ౯ࡍࡿ᪉ἲ (Kino and Kawakatu 2005; Ito et al. 2008)㸪ࡉࡽ࡟ࡣࢥࢡ࣮ࣥෆ࡛ࡢ ྛᡂศ㸦㟁Ꮚ㸪㝧㟁Ꮚ㸪㝧Ꮚ㸧ࡢศᅽ࠿ࡽ┦ᑐㄽⓗࢪ࢙ࢵࢺࡢ⤌ᡂ࡟ไ㝈ࢆࡘࡅࡿ᪉ἲࢆᥦၐࡋࡓࠋ(Kino, Kawakatu, Takahara 2012)ࠋᮏ◊✲࡛ࡣ㸪⭾ᙇࢥࢡ࣮ࣥຊᏛ࡟ࡼࡾ┿ࡢࢪ࢙ࢵࢺࣃ࣮࣡ࡀồࡵࡽࢀ࡚࠸ࡿ FRII ᆺ㟁Ἴ㖟Ἑ Cygnus A, 3C219,
3C223, 3C284 ࡟ᑐࡋ࡚㸪ྠᵝࡢ᪉ἲࢆ㐺ᛂࡋゎᯒࢆ⾜ࡗࡓࠋࡑࡢ⤖ᯝ㸪Cygnus A ࢆྵࡴ㸲ࡘࡢ FRII 㟁Ἴ㖟Ἑࡣ࢚ࢹ࢕ࣥࢺࣥගᗘ࡟༉ᩛࡍࡿࣃ࣡ࣇࣝ࡞ࢪ࢙ࢵࢺࢆᣢࡘ࡟ࡶ㛵ࢃࡽࡎ㸪࠸ࡎࢀࡢሙྜࡶ࣌࢔ࣉࣛࢬ࣐ࡀ ΰᅾࡍࡿࡇ࡜ࡀศ࠿ࡗࡓࠋࡘࡲࡾ㸪4 ኳయࡢࢪ࢙ࢵࢺ
⤌ᡂࡣ㟁Ꮚ࣭㝧Ꮚࣉࣛࢬ࣐ࡔࡅ࡛ࡣㄝ࡛᫂ࡁࡎ㸪㝧㟁ᏊࡢᏑᅾࢆ♧၀ࡍࡿࡶࡢ࡛࠶ࡿ
(Kawakatu, Kino, Takahara in preparation)ࠋ
࠙㸴ࠚ ࢲ࣮ࢡ࣐ࢱࣁ࣮ࣟࡢෆ㒊ᵓ㐀㸸ࢥ࢔࢝ࢫࣉၥ㢟Ᏹᐂࡢᵓ㐀ᙧᡂࡢࣃࣛࢲ࢖࣒㸪ࢥ࣮ࣝࢻࢲ࣮ࢡ࣐ࢱ࣮(CDM)ࢩࢼࣜ࢜ࡣ㸪 N యࢩ࣑࣮ࣗࣞࢩࣙࣥ࡟ࡼࡿ࡜ࢲ࣮ࢡ࣐ࢱ࣮(DM)ࣁ࣮ࣟ୰ᚰ㒊࡛㉁㔞ᐦᗘࡀⓎᩓࡍࡿ(࢝ࢫࣉ)ᵓ㐀ࢆணゝࡍࡿ(Navarro, Frenk & White 1997; Fukushige & Makino
1997)ࠋ ࡋ࠿ࡋ㸪ࡑࡢほ⤖ᯝ࡟ࡼࡿ࡜㸪▸ᑠ㖟Ἑࡢᐦᗘࡣ୰ᚰ㒊࡛Ⓨᩓࡏࡎ㸪୍ᐃ࡜࡞ࡿ(ࢥ࢔)ࡇ࡜ࡀሗ࿌ࡉࢀ࡚࠸ࡿ (Swaters et al. 2003; Spekkens et al.
2005; Oh et al. 2010)ࠋࡇࡢ⌮ㄽ࡜ほࡢ୙୍⮴ࡣ''ࢥ࢔—࢝ࢫࣉၥ㢟''࡜࿧ࡤࢀ㸪

CDM ࢩࢼࣜ࢜ࡢᮍゎỴၥ㢟ࡢ୍ࡘ࡛࠶ࡿࠋ௒ᅇᡃࠎࡣ㸪''㉸᪂ᫍ⇿Ⓨ࡟ࡼࡾ▸ᑠ㖟Ἑෆࡢ࢞ࢫࡀຍ⇕࣭⭾ᙇࡋ㸪ࡸࡀ࡚ᨺᑕ෭༷࣭཰⦰ࡀ㉳ࡇࡾ෌ࡧᫍᙧᡂࡀ㉳ࡇࡿ㸪࡜࠸࠺୍㐃ࡢ㐣⛬ࡢ⧞ࡾ㏉ࡋࡢ㔜ຊሙኚື࡟ࡼࡾ࢝ࢫࣉࡀࢥ࢔࡬࡜㑄⛣ࡍࡿ
࠿''ࢆ N యࢩ࣑࣮ࣗࣞࢩࣙࣥࢆ⏝࠸࡚ㄪ࡭ࡓࠋࡇࡇ࡛ࣂࣜ࢜ࣥࡢ㔜ຊሙࡣ࿘ᮇⓗ࡟᫬㛫ኚ໬ࡍࡿእሙ࡟ࡼࡗ࡚⾲⌧ࡋࡓࠋࡑࡢ⤖ᯝࣂࣜ࢜ࣥࡢ㔜ຊሙኚືࡢ᫬㛫ࢫࢣ࣮ࣝ࡟౫Ꮡࡋ࡚ DM ࣁ࣮ࣟ࡟ᙧᡂࡉࢀࡿࢥ࢔ࡢ኱ࡁࡉࡸ఩⨨ࡀ኱ࡁࡃኚ໬ࡍࡿ஦
ࡀࢃ࠿ࡗࡓࠋࡲࡓ㸪DM ࣁ࣮ࣟࡢ⢏Ꮚ⩌࡜እሙ㛫࡛㉳ࡇࡿඹ㬆ⓗ࡞⌧㇟࡟ᑐࡍࡿゎᯒⓗ࡞ࣔࢹࣝࢆᵓ⠏ࡋࡓࠋࡇࡢඹ㬆ࣔࢹࣝ࡟ࡼࡗ࡚㸪ࢥ࢔༙ᚄࡀ㔜ຊሙࡢ᫬㛫ኚື࿘ᮇ࡜㛵ಀࡀ࠶ࡿࡇ࡜ࢆ✺ࡁṆࡵࡓࠋ࠙㸵ࠚ ࢔ࣥࢻ࣓ࣟࢲࡢᾦ࡜ࡉࡊࡵࡁ

44

ᖹᡂ 24 ᖺᗘ ⟃Ἴ኱Ꮫ ィ⟬⛉Ꮫ◊✲ࢭࣥࢱ࣮ ᖺḟሗ࿌᭩㏆ᖺ㸪ࣁࢵࣈࣝᏱᐂᮃ㐲㙾ࡸࡍࡤࡿᮃ㐲㙾࡟௦⾲ࡉࢀࡿᆅୖ኱ᆺᮃ㐲㙾ࢆ᭱኱㝈ά⏝ࡋࡓ㏆ഐࡢ῝Ᏹᐂ᥈ᰝ࡟ࡼࡾ㸪⌧ᅾࡶ⥆ࡃ㖟Ἑ㐍໬ࡢ㐣⛬ࢆᇉ㛫ぢࡿࡇ࡜ࡀ࡛ࡁࡿࡼ࠺࡟࡞ࡗ࡚ࡁࡓࠋ࢔ࣥࢻ࣓ࣟࢲ㖟Ἑ࿘㎶࡟࠾࠸࡚ࡣ㸪࠾ࡧࡓࡔࡋ࠸ᩘ
ࡢᬯ࠸▸ᑠ㖟ἙࡀⓎぢࡉࢀࡿ࡜࡜ࡶ࡟㸪ࡑࢀࡽ▸ᑠ㖟Ἑࡢ⾪✺࡟ࡼࡿࡶࡢ࡜ᛮࢃ
ࢀࡿࢫࢸ࣮ࣛࢫࢺ࣮࣒ࣜࡸࢫࢸ࣮ࣛࢩ࢙ࣝ➼ࡢ⑞㊧ࡀ⥆ࠎ࡜᫂ࡽ࠿࡟ࡉࢀ࡚ࡁ࡚
࠸ࡿࠋ≉࡟࢔ࣥࢻ࣓ࣟࢲࡢᾦ㸦࢔ࣥࢻ࣓ࣟࢲࢫࢺ࣮࣒ࣜ㸧࡟㛵ࡋ࡚ࡣ㸪ほ࣭⌮ㄽࡢ୧㠃࠿ࡽࡢ◊✲ࡀ㐍ᒎࡋ࡚ࡁ࡚࠾ࡾ㸪㖟Ἑ⾪✺ࡢ㝿ࡢ㌶㐨㐠ືࡸࡑࡢ᫬ᮇ㸪⾪✺ࡋࡓ㖟Ἑࡢ㉁㔞ࡸ໬Ꮫ⤌ᡂ➼࡟ࡘ࠸࡚⌮ゎࡀ㐍ࢇ࡛ࡁ࡚࠸ࡿࠋᡃࠎࡣ㸪N య
ィ⟬࡜ 3 ḟඖࡢὶయຊᏛィ⟬ࢆ⤌ࡳྜࢃࡏࡓࣁ࢖ࣈࣜࢵࢻࢩ࣑࣮ࣗࣞࢩࣙࣥ࡟ࡼ
ࡾ㸪࢔ࣥࢻ࣓ࣟࢲ㖟Ἑࡢ෇┙࢞ࢫ࡜▸ᑠ㖟Ἑ࡟௜㝶ࡍࡿ࢞ࢫࡢὶయຊᏛⓗ࡞┦஫స⏝ࡢヲ⣽࡟ࡘ࠸࡚ㄪ࡭ࡓࠋ㖟Ἑ෇┙࢞ࢫ࡜▸ᑠ㖟Ἑ࢞ࢫࡢ┦஫స⏝࡟ࡼࡾⓎ⏕ࡍࡿ㖟Ἑ෇┙࢞ࢫࡢὶయຊᏛⓗ࡞ᣲື࡜㸪࢔ࣥࢻ࣓ࣟࢲࡢ෇┙࢞ࢫ࡛ほࡉࢀ࡚࠸ࡿࣜࣥࢢ≧ᵓ㐀ࡢ⏕ᡂ㐣⛬࡟ࡘ࠸࡚ヲ⣽࡞ゎᯒࢆ⾜ࡗࡓࠋࡲࡓ㸪▸ᑠ㖟Ἑࡢ㌶
㐨㐠ືࡢึᮇ᮲௳౫Ꮡᛶ࡟ࡘ࠸࡚኱つᶍࣃ࣓࣮ࣛࢱࢧ࣮࣋࢖ࢆ⾜࠸㸪ほࢆ෌⌧ࡍࡿ㌶㐨せ⣲ࢆồࡵࡓࠋ࠙㸶ࠚ 㖟Ἑࣁ࣮ࣟ୰ࢆ⁻࠺ᕧ኱ࣈࣛࢵࢡ࣮࣍ࣝ࡬ࡢ࢞ࢫ㝆╔࡜ࡑࡢᗈἼ㛗ᇦᨺᑕྛ㖟Ἑࡣࡑࢀࡒࢀࡢ୰ᚰ࡟ᕧ኱ࣈࣛࢵࢡ࣮࣍ࣝࢆᐟࡍࠋࡲࡓ㸪㖟Ἑࡣ࿘㎶ࡢ㖟Ἑ࡜⾪✺࣭ྜయࡋ㸪྾཰ྜేࡍࡿ஦࡛ࡑࡢ㉁㔞ࢆᡂ㛗ࡉࡏ࡚ࡁࡓ࡜⪃࠼ࡽࢀࡿࠋ
ࡇࢀࡽࡢ஦࠿ࡽ㸪㖟Ἑ⾪✺࡟ࡼࡾ⾨ᫍ㖟Ἑࡀቯࡉࢀࡓᚋࡋࡤࡽࡃࡢ㛫㸪ඖ⾨ᫍ㖟Ἑࡢ୰ᚰᕧ኱ࣈࣛࢵࢡ࣮࣍ࣝࡀぶ㖟Ἑࡢࣁ࣮ࣟ୰ࢆ⁻ࡗ࡚࠸ࡿ࡜ᮇᚅࡉࢀࡿࠋ㞄ࡢ㖟Ἑ࡛࠶ࡿ࢔ࣥࢻ࣓ࣟࢲ㖟Ἑࡣ㸪ࡇࡢ㖟Ἑ⾪✺࡟ࡼࡿ㖟Ἑ࡜ࣈࣛࢵࢡ࣮࣍ࣝࡢ
ඹ㐍໬ࢆ⌮ㄽ࡜ほࡢ୧㠃࠿ࡽ⌮ゎࡍࡿୖ࡛㸪᭱ୖࡢᐇ㦂ሙ࡛࠶ࡿࠋヲ⣽࡞ほ࡜ᩘ್ᐇ㦂ࡢẚ㍑࡟ࡼࡾ㸪⣙ 10 ൨ᖺ᫇࡟⾨ᫍ㖟Ἑࡀ⾪✺ࡋ㸪௒⌧ᅾ㸪ඖ⾨ᫍ㖟Ἑࡢ◚∦ࡀ࢔ࣥࢻ࣓ࣟࢲ㖟Ἑ࿘㎶࡟⑞㊧࡜ࡋ࡚ṧࡗ࡚࠸ࡿ஦ࡀࢃ࠿ࡗ࡚࠸ࡿࠋࡇࡢ
ඖ⾨ᫍ㖟Ἑࡢ୰ᚰᕧ኱ࣈࣛࢵࢡ࣮࣍ࣝࡀ㸪ࣁ࣮ࣟࡢᕼⷧ࢞ࢫࢆ Bondi 㝆╔࡟ࡼࡾ྾࠸㎸ࡴ᫬࡟ᙧᡂࡉࢀࡿ㝆╔෇┙ࡢᗈἼ㛗ᇦᨺᑕࢆィ⟬ࡋࡓࠋᵝࠎ࡞᳨ฟ⿦⨨ࡢឤᗘ࡜ẚ㍑ࡋࡓ࡜ࡇࢁ㸪㟁Ἴ㡿ᇦࡢ᪤Ꮡ⿦⨨࡛༑ศ᳨ฟྍ⬟࡛࠶ࡿ஦ࡀࢃ࠿ࡗࡓࠋ
࠙㸷ࠚ Ᏹᐂㄽⓗ㖟Ἑᙧᡂࢩ࣑࣮ࣗࣞࢩࣙࣥ

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ᖹᡂ 24 ᖺᗘ ⟃Ἴ኱Ꮫ ィ⟬⛉Ꮫ◊✲ࢭࣥࢱ࣮ ᖺḟሗ࿌᭩࢞ࢫࡢ෭༷ࡸᫍᙧᡂ, ㉸᪂ᫍ⇿Ⓨ➼ࡢ≀⌮㐣⛬ࢆྲྀࡾධࢀࡓᏱᐂㄽⓗ㖟Ἑᙧᡂࢩ࣑࣮ࣗࣞࢩࣙࣥࢆ⏝࠸࡚௨ୗࡢࡼ࠺࡞◊✲ࢆ⾜ࡗࡓ (i) 㐲᪉Ᏹᐂࡢᫍᙧᡂ㖟Ἑ࡛࠶ࡿࣛࢧࣈ࣑ࣜἼ࡛᫂ࡿࡃ㍤ࡃࢧࣈ࣑ࣜ㖟Ἑࡢ≀⌮ⓗᛶ㉁ࢆ᫂ࡽ࠿࡟ࡋࡓ
(Shimizu et al. 2012ab). (ii) 㖟Ἑ⣔ࢧ࢖ࢬࡢ㖟Ἑࢆ㧗ศゎ⬟࡞Ᏹᐂㄽⓗࢩ࣑࣮ࣗࣞࢩ࡛ࣙࣥᙧᡂࡋ, 㖟Ἑ⣔ࣂࣝࢪࡢᙧᡂ࡟ࡘ࠸࡚ㄪ࡭ࡓ. ᨃࣂࣝࢪ࡜࿧ࡤࢀࡿᵓ
㐀ࡀ௒ࡲ࡛⪃࠼ࡽࢀ࡚࠸ࡓࡼ࠺࡞෇┙ࡢỌᖺ㐍໬࡛ࡣ࡞ࡃ㧗㉥᪉೫⛣ࡢ⇿Ⓨⓗᫍᙧᡂ࡛ᙧᡂࡉࢀࡿ࡜࠸࠺᪂ࡋ࠸ᥥീࢆᥦ᱌ࡋࡓ (Okamoto 2013). ࡲࡓ, ᵝࠎ࡞ࢢ࣮ࣝࣉ㛫࡛ࡢ㖟Ἑᙧᡂࣔࢹࣝࢆẚ㍑ࡍࡿࣉࣟࢪ࢙ࢡࢺ࡟ࡶཧຍࡋࡓ
(Scannapieco et al. 2012).

࠙㸯㸮ࠚ

6 ḟඖ఩┦✵㛫ୖࡢ Vlasov-Poisson ࢩ࣑࣮ࣗࣞࢩࣙࣥ

↓⾪✺⮬ᕫ㔜ຊ⣔ࡢᩘ್ࢩ࣑࣮ࣗࣞࢩ࡛ࣙࣥࡣ㸪ࡇࢀࡲ࡛ N యࢩ࣑࣮ࣗࣞࢩࣙࣥࡀᖜᗈࡃ
⏝࠸ࡽࢀ࡚ࡁࡓࡀࢽ࣮ࣗࢺࣜࣀ࡞࡝ࡢ㏿ᗘศᩓࡀ኱ࡁ࠸ᡂศࡢ↓⾪✺ῶ⾶ࢆṇ☜࡟ྲྀࡾᢅ࠺࡟ࡣ୙ྥࡁ࡛࠶ࡗࡓࠋࡇࡢ N యࢩ࣑࣮ࣗࣞࢩࣙࣥࡢᙅⅬࢆඞ᭹ࡍࡿᡭἲ࡜ࡋ࡚ 6 ḟඖ఩┦✵㛫ୖ࡛ࡢ↓⾪✺࣎ࣝࢶ࣐ࣥ᪉⛬ᘧࢆ᭷㝈య✚ἲ࡟ࡼࡗ࡚┤᥋ᩘ್ࢩ࣑࣮ࣗࣞࢩࣙࣥࡍ
ࡿᡭἲࢆୡ⏺࡛ึࡵ࡚㛤Ⓨࡋࡓࠋᮏᖺᗘࡣ㸪Ᏹᐂㄽⓗ࡞኱つᶍᵓ㐀ᙧᡂࡢᩘ್ࢩ࣑࣮ࣗࣞ
ࢩࣙࣥ࡟ᛂ⏝࡛ࡁࡿࡼ࠺࡟ඹືᗙᶆ⣔࡛ࡢ↓⾪✺࣎ࣝࢶ࣐ࣥ᪉⛬ᘧࡢᩘ್ゎἲࢆ㛤Ⓨࡋࡓࠋ࠙㸯㸯ࠚ GPU ࢆ฼⏝ࡋࡓ㍽ᑕ㍺㏦ࢩ࣑࣮ࣗࣞࢩࣙࣥࢥ࣮ࢻࡢ㛤Ⓨ㍽ᑕ㍺㏦ࡣᏱᐂ≀⌮Ꮫࡢᩘ್ࢩ࣑࣮ࣗࣞࢩࣙࣥ࡟࠾࠸࡚㔜せ࡞ᙺ๭ࢆᯝࡓࡍࡀ㸪ከᩘࡢග※࠿ࡽࡢ㍽ᑕ㍺㏦ィ⟬ࡣィ⟬ࢥࢫࢺࡀ⭾኱࡜࡞ࡾ㸪኱つᶍ࡞ィ⟬ࡸὶయຊᏛ࡜⤌ࡳྜࢃࡏࡓ㍽ᑕὶయィ⟬ࡢᐇ⾜ࡣᅔ㞴࡛࠶ࡗࡓࠋᡃࠎࡣከᩘࡢග※࠿ࡽ
ࡢ㍽ᑕ㍺㏦ࢆ㧗㏿࡟ィ⟬ࡍࡿ ARGOT (accelerated radiation transfer on grids
using oct tree) ἲࢆ GPU ࢆ⏝࠸࡚ࡉࡽ࡟㧗㏿໬ࡍࡿࡇ࡜࡟ᡂຌࡋࡓࠋࡲࡓ㸪GPU
ࢆᦚ㍕ࡋࡓ኱つᶍࢡࣛࢫࢱ࣮ࢩࢫࢸ࣒࡛࠶ࡿ HA-PACS ୖ࡛ࣀ࣮ࢻ୪ิ໬ࢆ⾜ࡗ
ࡓࠋ

࠙㸯㸰ࠚ

AGN ࡢ㍽ᑕ࡟ࡉࡽࡉࢀࡓศᏊ㞼ࡢ㐍໬࡟ࡘ࠸࡚ࡢ◊✲άື㖟Ἑ᰾(AGN)ࡣ㸪Ᏹᐂ࡛᭱ࡶ᫂ࡿ࠸ኳయࡢ 1 ࡘ࡛࠶ࡾ㸪ࡑࡢගᗘࡣ㖟Ἑᮏయ࡟༉ᩛ
ࡍࡿࠋගࡢ኱㒊ศࡣ㸪㟁㞳⬟ຊࢆᣢࡗࡓ⣸እග㸪ཬࡧ㸪X ⥺ࡢἼ㛗ᖏ࡛ᨺᑕࡉࢀࡿࡓࡵ㸪ẕ㖟Ἑࡢ㐍໬࡟኱ࡁ࡞ᙳ㡪ࢆ୚࠼ࡓ࡜୍⯡࡟⪃࠼ࡽࢀ࡚࠸ࡿࠋࡋ࠿ࡋ㸪AGN ࡢάືᛶࡢヲ⣽ࡀ࡝ࡢࡼ࠺࡟Ỵᐃࡉࢀࡿ࠿ࡣ᫂ࡽ࠿࡛࡞࠸ࠋࡑࡇ࡛㸪ᮏ◊✲࡛ࡣ㸪AGN ⌧㇟ࡢᣢ⥆ᛶࡢ⌮ゎࢆ㐍ࡵࡿࡇ࡜ࢆ┠ⓗ࡜ࡋ࡚㸪࢞ࢫ౪⤥࡟㔜せ࡞ᙺ๭ࢆᯝࡓࡍ࡜ᮇᚅࡉࢀࡿගᏛⓗ࡟ཌ࠸ศᏊ㞼ࡢ㍽ᑕὶయィ⟬ࢆ⾜ࡗࡓࠋࡑࡢ⤖ᯝ㸪ศᏊ㞼⾲㠃࡛ࡢ㟁㞳ࣃ࣓࣮ࣛࢱࡢ኱ࡁࡉ࡟ᛂ

46

ᖹᡂ 24 ᖺᗘ ⟃Ἴ኱Ꮫ ィ⟬⛉Ꮫ◊✲ࢭࣥࢱ࣮ ᖺḟሗ࿌᭩ࡌ࡚㸪ศᏊ㞼ࡢ㐍໬ࡣ 2 ✀㢮࡟኱ูࡉࢀࡿࡇ࡜ࡀࢃ࠿ࡗࡓࠋ㟁㞳ࣃ࣓࣮ࣛࢱࡀᙅ࠸ሙྜ࡟
ࡣ㸪ศᏊ㞼ࡣ⌫ᑐ⛠ⓗ࡞ග⵨Ⓨ࡟ࡼࡗ࡚㉁㔞ࢆኻ࠸࡞ࡀࡽ㸪ࡑࡢ཯స⏝࡟ࡼࡿᅽຊ࡛㸪ศᏊ㞼ࡢ୍㒊ࡀ㔜ຊᔂቯ࡟⮳ࡿࠋ㟁㞳ࣃ࣓࣮ࣛࢱࡀᙉ࠸ሙྜ࡟ࡣ㸪㍽ᑕᅽࡀຠᯝⓗ࡟࡞ࡾࡣࡌࡵ㸪ග⵨ⓎὶࡢศᏊ㞼⾲㠃࡟㛢ࡌ㎸ࡵ࡞ࡀࡽ㸪ศᏊ㞼ᢲࡋࡘࡪࡋ㸪᭱⤊ⓗ࡟ࡣศᏊ㞼ࡢ୍㒊ࢆ㔜ຊᔂቯࡉࡏࡿࡇ࡜ࡀࢃ࠿ࡗࡓࠋ

࠙㸯㸱ࠚᴟ㧗ගᗘ X ⥺※ࡢ୰㛫㉁㔞ࣈࣛࢵࢡ࣮࣍ࣝೃ⿵
୰㛫㉁㔞ࣈࣛࢵࢡ࣮࣍ࣝ(BH)ࡢ᭱᭷ຊೃ⿵࡛࠶ࡿᴟ㧗ගᗘ X ⥺※(Hyper
Luminous X-ray source)࡟ࡘ࠸࡚㸪X ⥺ࢫ࣌ࢡࢺࣝࢆ㝆╔෇┙ࣔࢹࣝࢆ⏝࠸࡚ゎ
ᯒࡋ㸪BH ㉁㔞ࢆ᥎ᐃࡋࡓࠋ
ᴟ㧗ගᗘ X ⥺※ ESO243-49 HLX-1 ࡣ㸪㏆ഐࡢ෇┙㖟Ἑ(㉥᪉೫⛣ z = 0.02) ࡢ෇┙㠃ୖ✵࡟෗ࡗ࡚࠾ࡾ㸪㉥᪉೫⛣♧၀ࡉࢀ࡚࠸ࡿࠋࡇࡢ㊥㞳ᐃࡢヨࡳ࠿ࡽࡇࡢ㖟Ἑ࡜ྠࡌ㊥㞳࡟ᒃࡿ஦ࡀ

ᐃࡀṇࡋࡅࢀࡤ㸪X ⥺ගᗘࡣ 1042 erg/s ࡟㐩ࡋ㸪㉸㧗ගᗘ X ⥺※ (Ultra Luminous X-ray source)ࡼࡾࡶ 1 ᱆௨ୖ᫂ࡿࡃ㸪୰㛫㉁㔞
BH ࡢ᭱᭷ຊೃ⿵࡛࠶ࡿࠋ୰㛫㉁㔞 BH ࡣᐇᅾࡍࡿ࠿㸪ࡑࡢ㉳※ࡣఱ࠿㸪ඖ⾨ᫍ㖟Ἑࡢ୰ᚰ BH ࡀᾋ㐟ࡋ࡚࠸ࡿࡢ࠿㸪ᕧ኱ BH ࡢ✀࡞ࡢ࠿➼ࡢ␲ၥ࡟ᣮࡴ⤯ዲࡢᐇ㦂ሙ࡜ゝ࠼ࡿࠋ
ࡇࢀࡲ࡛ࡢ HLX-1 ࡢ X ⥺ࢫ࣌ࢡࢺࣝࢆ㝆╔෇┙ࣔࢹࣝࢆ⏝࠸࡚ゎᯒࡍࡿ◊✲࡛ࡣ㸪ள⮫⏺㝆╔⋡࡟㝈ᐃࡉࢀࡿᶆ‽㝆╔෇┙ࣔࢹࣝࢆᇶ࡟ࡋ࡚࠸ࡓࠋࡋ࠿ࡋ㸪኱ගᗘኳయ࡟ள⮫⏺㝆╔ࢆ௬ᐃࡋ࡚ BH ㉁㔞ࢆ᥎ᐃࡋ୰㛫㉁㔞࡜࠸࠺⟅࠼ࢆᚓࡿ஦ࡣ㸪௬ᐃࡀ⤖ㄽ࡟┤⤖ࡋ࡚࠸ࡿ༴㝤ᛶࡀ࠶ࡿࠋ
ࡑࡇ࡛㸪ள⮫⏺࠿ࡽ㉸⮫⏺㝆╔⋡ࡲ࡛ᖜᗈࡃ࢝ࣂ࣮ࡍࡿࡇ࡜࡛㝆╔⋡࡟஦๓ࡢ௬ᐃࢆᚲせ࡜ࡏࡎ㸪⛣ὶ࣭┦ᑐㄽⓗຠᯝ෇┙⾲ᒙ࡛ࡢࢥࣥࣉࢺࣥᩓ஘ࢆྵࢇࡔ෇┙ࢫ࣌ࢡࢺࣝࣔࢹࣝ(Kawaguchi 2003)ࢆ 10 ୓ኴ㝧㉁㔞ࡲ࡛ࡢ BH ࡟ᑐࡋ࡚ィ⟬ࡋࡓࠋ
3 ᖺ࡟Ώࡗ࡚⣙ 30 ಸගᗘࡀ᫬㛫ኚືࡍࡿ HLX-1 ࡢከ᫬้ X ⥺ࢫ࣌ࢡࢺࣝࢆゎᯒࡋࡓ࡜ࡇࢁ㸪⣙ 1.8 ୓ኴ㝧㉁㔞 BH ࡬ࡢ࢞ࢫ㝆╔࡟ࡼࡗ࡚ࢹ࣮ࢱࢆㄝ࡛᫂ࡁࡿ஦
ࡀࢃ࠿ࡗࡓࠋ࠙㸯㸲ࠚ

AVX ࿨௧∧ Phantom-GRAPE
2011 ᖺ࡟࣮ࣜࣜࢫࡉࢀࡓ Intel ࡢ᪂ᆺࣉࣟࢭࢵࢧ Sandy-Bridge ࡛᪂ࡓ࡟ᐇ⿦ࡉ

ࢀ ࡓ SIMD (Single-Instruction-Multi-Data) ࿨ ௧ ࡛ ࠶ ࡿ Advanced Vector
eXtension (AVX) ࿨ ௧ ࢭ ࢵ ࢺ ࢆ ⏝ ࠸ ࡓ 㸪 㔜 ຊ ከ య ᩘ ್ ィ ⟬ ࣛ ࢖ ࣈ ࣛ ࣜ
Phantom-GRAPE ࢆ㛤Ⓨࡋ㸪ࡇࢀࡲ࡛ࡢ SIMD ࿨௧࡛࠶ࡿ Streaming SIMD
Extension (SSE)࿨௧ࢭࢵࢺࢆ⏝࠸ࡓࡶࡢࡼࡾࡶࡼࡾ㧗㏿࡞₇⟬ࢆᐇ⌧ࡋࡓࠋ

47

ᖹᡂ 24 ᖺᗘ ⟃Ἴ኱Ꮫ ィ⟬⛉Ꮫ◊✲ࢭࣥࢱ࣮ ᖺḟሗ࿌᭩

Phantom-GRAPE ࡣ㸪4 ḟ࢚࣑࣮ࣝࢺ✚ศࢆ㌶㐨ィ⟬࡟⏝࠸ࡿ㧗⢭ᗘ࡞⾪✺⣔㔜ຊከయ⏝࡜㸪㖟Ἑࡸ㖟Ἑᅋ࡞࡝ࡢ↓⾪✺⣔⏝ࡢ 2 ✀㢮ࢆ㛤Ⓨࡋ㸪Google Code ࡛බ㛤ࡋ࡚࠶ࡿࠋ࠙㸯㸳ࠚᫍ㛫✵㛫࡟࠾ࡅࡿ࢔࣑ࣀ㓟ࡢ෇೫ගἼㄏ㉳㙾ീ␗ᛶయ㐣๫ࡢ⌮ㄽⓗ◊✲㸦Ᏹᐂ࣭⏕࿨࣭≀ᛶ࣭ཎᏊ᰾ศ㔝㐃ᦠ㸧⏕࿨యࡢᇶᮏศᏊ࡟࢔࣑ࣀ㓟ࡀ࠶ࡿࡀ㸪ᐇ㦂ᐊ࡛࢔࣑ࣀ㓟ࢆసᡂࡍࡿ࡜㸪ᕥᕳࡁ㸦L ᆺ㸧࡜ྑᕳࡁ㸦D ᆺ㸧ࡀྠ㔞⏕ᡂࡉࢀࡿࡀ㸪ᆅ⌫ୖࡢ⏕࿨࡛ࡣ࡯࡜ࢇ࡝ L ᆺ࢔࣑ࣀ㓟ࡋ࠿౑ࢃࢀ࡚࠸࡞࠸ࠋࡇࢀࢆ㸪㙾ീ␗ᛶయ㐣๫࡜࠸࠺ࠋ1969 ᖺ㸪࣮࢜ࢫࢺࣛࣜ࢔ࡢ࣐࣮ࢳࢯࣥᮧ࡟㝹▼ࡀⴠୗࡋ㸪ࡑࡢ㝹▼࠿ࡽ࢔࣑ࣀ㓟ࡀ᳨ฟࡉࢀࡓࠋࡑ
ࡋ࡚㸪ࢃࡎ࠿࡛ࡣ࠶ࡿࡀ㙾ീ␗ᛶయ㐣๫ࡀⓎぢࡉࢀࡓࠋ2010 ᖺ࡟ࡣ㸪㉸㧗ࡢ㝹▼࠿ࡽ࢔࣑ࣀ㓟ࡀⓎぢࡉࢀ㸪㝹▼ࡢ࢔࣑ࣀ㓟ࡣᆅ⌫࡟኱Ẽᅪ㏻㐣ࡢ㝿࡟ኚᡂࡍࡿࡇ
࡜࡞ࡃⴠୗࡍࡿࡇ࡜ࡀศ࠿ࡗࡓࠋⓎぢࡉࢀࡓ㙾ീ␗ᛶయ㐣๫ࡣࢃࡎ࠿࡞ࡶࡢ࡛࠶ࡿ
ࡀ㸪ᐇ㦂ࢆࡍࡿ࡜㙾ീ␗ᛶయ㐣๫ࡣ⮬ᕫゐ፹཯ᛂ࡟ࡼࡾᛴ㏿࡟ቑ኱ࡍࡿࡇ࡜ࡀศ࠿
ࡗ࡚ࡁࡓࠋࡼࡗ࡚㸪࢔࣑ࣀ㓟ࡢ㙾ീ␗ᛶయ㐣๫ࡀᏱᐂ✵㛫࡛㉳ࡇࡾ㝹▼ࢆ㏻ࡌ࡚ᆅ⌫࡟㐠ࡤࢀ㸪ࡑࢀࡀᆅୖ࡛ᛴ㏿࡟ቑᖜࡋࡓྍ⬟ᛶࡀ࠶ࡿࠋࡲࡓ㸪ᐇ㦂ᐊ࡛෇೫ගࡢ
ගࢆᙜ࡚ࡿ࡜㙾ീ␗ᛶయ㐣๫ࡀᘬࡁ㉳ࡇࡉࢀࡿࡇ࡜ࡀศ࠿ࡗ࡚ࡁࡓࠋࡑࡋ࡚㸪㏆ᖺ࡟࡞ࡗ࡚㸪࢜ࣜ࢜ࣥᗙࡢᫍᙧᡂ㡿ᇦ(OMC-1)࡛෇೫ගἼࡀⓎぢࡉࢀࡓࠋࡼࡗ࡚㸪ཎጞ⣔ࡢ㏆ࡃ࡛኱㉁㔞ᫍࡀㄌ⏕ࡋࡓ࡜ࡍࢀࡤ㸪ኴ㝧⣔ෆ࡛࢔࣑ࣀ㓟ࡢ㙾ീ␗ᛶయ㐣๫ࡀ㉳ࡇࡗࡓྍ⬟ᛶࡀ࠶ࡿࠋ௨ୖࡢ஦ᐇࢆ⫼ᬒ࡟㸪Ᏹᐂ✵㛫࡛෇೫ගἼ࠿ࡽ࢔࣑ࣀ㓟ࡢ㙾ീ␗ᛶయ㐣๫ࢆᘬࡁ㉳ࡇࡍ㐣⛬࡟ࡘ࠸࡚ࡢ㔞Ꮚከయィ⟬ࢆ㐍ࡵ࡚࠸ࡿࠋᡃࠎࡣ㸪෇೫ගἼ྾཰࡜࢔࣑ࣀ㓟ࡢගບ㉳࡟ࡼࡿᔂቯ࣭ᨵኚ཯ᛂࡢ㐣⛬ࢆゎᯒࡋࡓࠋ➨୍ཎ⌮ィ⟬࡟ࡼࡾ㸪┿✵୰࡟࠾ࡅࡿ࢔࣑ࣀ㓟ࡢ᭱Ᏻᐃᵓ㐀ࢆồࡵ㸪ࡑࡢග྾཰ᛶ࡜෇೫
ග஧Ⰽᛶࡢ್ࢆồࡵࡓࠋࡑࡢ⤖ᯝ㸪࢔࣑ࣀ㓟ࡢග≀ᛶࡣࡑࡢ✀ࡢ≉ᚩ࡜࡞ࡿഃ㙐ࡼࡾ࢔࣑ࣀ㓟඲య࡟ඹ㏻ࡍࡿ୺㙐ࡢᵓ㐀࡟ࡼࡾᙉࡃ౫Ꮡࡋ㸪Ἴ㛗ᖏ࡜ࡋ࡚ࣛ࢖࣐ࣥ ᖏࡢගࡀ㔜せ࡛࠶ࡿࡇ࡜ࢆ᫂ࡽ࠿࡟ࡋࡓࠋ

࠙㸯㸴ࠚ⣔እᝨᫍ࡟࠾ࡅࡿࣂ࢖᳨࣐࣮࣮࢜࢝ฟࢆ┠ᣦࡋࡓගྜᡂ࢔ࣥࢸࢼᶵᵓࡢ

࢚ࢿࣝࢠ࣮⛣ືィ⟬㸦Ᏹᐂ࣭⏕࿨ศ㔝㐃ᦠ㸧᥈ᰝᶵ Kepler ࡟ࡼࡗ࡚ኴ㝧⣔እᝨᫍࡢᩘࡣ኱ࡁࡃ㏣ຍࡉࢀ࡚࠾ࡾ, ᆅ⌫ᆺᝨᫍࡸࣁࣅࢱ
ࣈࣝࢰ࣮ࣥෆ࡟ධࡿᝨᫍࡢほ࡟ࡶᡂຌࡋ࡚࠸ࡿࠋᆅ⌫࡟㢮ఝࡋࡓᝨᫍࡢⓎぢࡀᮇᚅࡉࢀ

ࡿ୰࡛, ᚓࡽࢀࡿࢫ࣌ࢡࢺࣝ࠿ࡽ⏕࿨ࡢ⑞㊧࡛࠶ࡿࣂ࢖࣐࣮࣮࢜࢝ࢆዴఱ࡟᳨ฟࡍࡿ࠿ࡀ
ㄢ㢟࡟࡞ࡗ࡚࠸ࡿࠋᆅ⌫ࡢ⏕࿨ࡢ㐍໬࡟࠾࠸࡚ගྜᡂࡣᴟࡵ࡚㔜せ࡛࠶ࡾ, ගྜᡂࡢ⑞㊧ࡢ48

ᖹᡂ 24 ᖺᗘ ⟃Ἴ኱Ꮫ ィ⟬⛉Ꮫ◊✲ࢭࣥࢱ࣮ ᖺḟሗ࿌᭩

୰࡛ࡶ 750nm ௜㏆ࡢ㏆㉥እ㡿ᇦ࡟ぢࡽࢀࡿ཯ᑕࢫ࣌ࢡࢺࣝࡢ≉ᚩⓗ࡞໙㓄㸦red edge㸧ࡣ᭷ຊ࡞ࣂ࢖࣐࣮࣮࢜࢝࡜࡞ࡾᚓࡿࠋᵝࠎ࡞ࢫ࣌ࢡࢺࣝᆺࡢ୺ᫍࢆබ㌿ࡍࡿ⣔እᝨᫍ࡟࠾࠸
࡚ගྜᡂ⏕≀ࡢᏑᅾࢆ᝿ᐃࡋࡓሙྜ, ගᤕ㞟ࡢᙧែࡀ኱ࡁࡃ␗࡞ࡿ࡜⪃࠼ࡽࢀࡿࠋᆅ⌫ࡢගྜᡂ⏕≀ࡢሙྜࡣ୺࡛ᫍ࠶ࡿኴ㝧ࡢࢫ࣌ࢡࢺࣝẚࡢගࢆຠ⋡Ⰻࡃᤕ㞟ࡍࡿࡼ࠺࡟㐍໬ࡋ࡚᮶ࡓ࡜⪃࠼ࡿ࡭ࡁ࡛࠶ࡾ, ࢡࣟࣟࣇ࢕ࣝ࡞࡝ࡢගྜᡂⰍ⣲࠿ࡽ࡞ࡿ࢔ࣥࢸࢼ⣔ࡣ⎔ቃ࡟ࡼࡗ࡚Ⰽ⣲ࡢ✀㢮ࡸ㓄⨨࡞࡝ࡢᙧែࡀ␗࡞ࡿࠋගࢆཷࡅࡓⰍ⣲ࡣ㟁Ꮚບ㉳ࡉࢀ, ㏆ࡃࡢⰍ⣲࡟㟁Ꮚ≧ែࢆ⛣ືࡉࡏࡿ࡜࠸࠺㐣⛬ࢆ㏻ࡌ࡚ຠ⋡ⓗ࡟ග࢚ࢿࣝࢠ࣮ࢆ໬Ꮫ࢚ࢿࣝࢠ࣮࡟ኚ᥮
ࡍࡿࠋ⣔እᝨᫍ࡟࠾࠸࡚ࡣ␗࡞ࡿගᤕ㞟ࡢᙧែࢆྲྀࡿሙྜ, ࡑࢀ࡟ᑐᛂࡋࡓἼ㛗ᇦ࡟ගྜᡂ
ࡢ඙ೃࢆ♧ࡍྍ⬟ᛶࡀ࠶ࡿࠋᡃࠎࡣ㸪⣔እᝨᫍࡢගࡢࢫ࣌ࢡࢺࣝẚ࡜᳜≀ࡢගᤕ㞟ࡢᙧែ࡜ࡢ┦㛵࡟ࡘ࠸࡚ᐃ㔞ⓗᣦᶆࢆᑟฟࡍࡿࡇ࡜ࢆ┠ⓗ࡟㸪ගᤕ㞟⣔ࡢ㔞Ꮚ໬Ꮫィ⟬ࢆ⾜ࡗࡓࠋ࢔ࣥࢸࢼࢆᵓᡂࡍࡿⰍ⣲ 1 ࡘ 1 ࡘࡢບ㉳ ≧ែࢆ᫬㛫౫Ꮡᐦᗘỗ㛵ᩘἲ࡟ࡼࡾィ⟬ࡋ, Ⰽ⣲㛫࡛ࡣ཮ᴟᏊ-཮ᴟᏊ┦஫స⏝ࡍࡿ㏆ఝࣔࢹࣝ ࢆᵓ⠏ࡋࡓࠋࡲࡓ, ධᑕග࡜ࡋ࡚࠶ࡿ᣺ືᩘ
ࡢ㟁ሙࢆ༳ຍࡋ࡚⣔ࡢ㔞ᏊຊᏛⓗ᫬㛫Ⓨᒎࢆ㏣㊧ࡍࡿࡇ࡜࡟ࡼࡗ࡚ࢫ࣌ࢡࢺࣝᙉᗘࢆ⟬ฟࡋࡓࠋࡇࢀ࡟ࡼࡾ㸪࢔ࣥࢸࢼ⣔ࡢᙧែ࡜ red edge ࡜ࡢ┦㛵ࢆㄪ࡭, ⣔እᝨ࡛ᫍ᝿ᐃࡉࢀࡿ
ࢫ࣌ࢡࢺࣝࢆ㆟ㄽࡋࡓࠋ4.

ᩍ⫱࠙Ꮫ఩ㄽᩥࠚ
㸺༤ኈㄽᩥ㸼
1. Mohammad Ali Nawaz
Interaction of Jets with the Intracluster Medium
2. Marc White
Outflows from Young Stellar Objects㸺ಟኈㄽᩥ㸼
㸯㸬Ᏻ㒊 ∾ே
3 ḟඖ㍽ᑕὶయィ⟬࡟ࡼࡿ⣸እ⥺㍽ᑕሙ୰ࡢᫍᅋᙧᡂ㐣⛬ࡢ◊✲㸰㸬஬༑ᔒ ᮒኟ⌫ᑐ⛠ᐃᖖ㖟Ἑ㢼ࡢゎᯒ㸱㸬኱㔝 ⣧ GPU ࢆ⏝࠸ࡓ㍽ᑕὶయຊᏛࢩ࣑࣮ࣗࣞࢩࣙࣥࡢ㧗㏿໬㸲㸬ஂಖ⏣ ᫂ኟ ึ௦ᫍᙧᡂ࡟࠾ࡅࡿ⣸እ⥺㍽ᑕࡢὶయຊᏛⓗຠᯝ49

ᖹᡂ 24 ᖺᗘ ⟃Ἴ኱Ꮫ ィ⟬⛉Ꮫ◊✲ࢭࣥࢱ࣮ ᖺḟሗ࿌᭩㸺Ꮫኈㄽᩥ㸼㣤ሯ ᐇ⣚⣔እᝨᫍ⣔࡟࠾ࡅࡿ㌶㐨஺ᕪ࡟ࡼࡿ࣍ࢵࢺࢪࣗࣆࢱ࣮ᙧᡂ
࠙㞟୰ㅮ⩏ࠚ࣭ᱵᮧ 㞞அ
ࠕ㍽ᑕ㍺㏦࣭㍽ᑕὶయຊᏛࠖ㸦2012 ᖺ 7 ᭶ 19 ᪥㸪༓ⴥ኱Ꮫ㸪༓ⴥᕷ㸧࣭ᒸᮏ ᓫࠕ㖟Ἑᙧᡂ࡜ࢲ࣮ࢡ࣐ࢱ࣮ࠖ➨ 7 ᅇ ⣲᰾Ᏹᐂ⼥ྜ ࣞࢡࢳ࣮ࣕ ࢩ࣮ࣜࢬ (2012 ᖺ 11 ᭶ 20
᪥ࠥ2012 ᖺ 11 ᭶ 21 ᪥, ⚄ᡞ኱Ꮫ, ⚄ᡞᕷ)5.

ཷ㈹㸪እ㒊㈨㔠㸪▱ⓗ㈈⏘ᶒ➼㸯㸧࠙ཷ㈹ࠚ
ձACM Gordon Bell Prize㸪▼ᒣᬛ᫂㸪 4.45 Pflops Astrophysical N-Body
Simulation
on K computer – The Gravitational Trillion-Body Problem, 2012 ᖺ 11 ᭶ 16
᪥
ղHPCS IEEE Computer Society Japan Chapter ඃ⚽ⱝᡭ◊✲㈹㸪ᡪ㇂㇦㸪㔜ຊከయ⣔⏝ Tree Code ࡢ୪ิ GPU ໬࡟ࡼࡿィ⟬ຍ㏿㸪2013 ᖺ 1 ᭶ 16 ᪥㸰㸧࠙እ㒊㈨㔠ࠚ㸺௦⾲⪅㸼࣭ᇶ┙◊✲㸦㹑㸧㸸ᱵᮧ 㞞அ㸦௦⾲⪅㸧㸦2008 ᖺᗘ᥇ᢥ㸪⥅⥆㸧 ࠕ➨୍ୡ௦ኳయ࠿ࡽཎጞ㖟Ἑ࡟⮳ࡿᏱᐂᬯ㯮᫬௦ࡢゎ᫂ࠖ (880 ୓෇)࣭ᇶ┙◊✲㸦㸿㸧㸸᳃ ṇኵ 㸦௦⾲⪅㸧 㸦⥅⥆㸧 ࠕ⌮ㄽ࡜ほࡢ⼥ྜ࡟ࡼࡿ㖟ἙⓎ⏕Ꮫࡢ᥈ồࠖ (560 ୓෇)࣭ ࣉࣞᡓ␎࢖ࢽࢩ࢔ࢸ࢕ࣈ㸸᳃ ṇኵ 㸦௦⾲⪅㸧㸦⥅⥆㸧 ࠕ࢔ࢡࢭ࣮ࣛࣞࢱ࡟ࡼࡿ㖟Ἑ㍽ᑕὶయຊᏛࡢᖥ㛤ࡅࠖ(500 ୓෇)࣭⛉◊㈝ⱝᡭ◊✲㸦㹀㸧:ᒸᮏ ᓫ (௦⾲⪅) (᪂つ)ࠕ㍽ᑕὶయࢩ࣑࣮ࣗࣞࢩࣙࣥࢆ⏝࠸ࡓ㖟Ἑ㢼㥑ືᶵᵓࡢゎ᫂ࠖ(110 ୓෇)࣭⛉◊㈝ⱝᡭ◊✲㸦㹀㸧:㛗㇂ᕝ ㈼஧㸦௦⾲⪅㸧㸦᪂つ㸧(210 ୓෇)ࠕᏱᐂㄽⓗ㍽ᑕࢩ࣑࣮ࣗࣞࢩ࡛ࣙࣥゎ᫂ࡍࡿᏱᐂ෌㟁㞳ᮇࡢ㖟Ἑᙧᡂྐ࣭ࠖ⛉◊㈝ⱝᡭ◊✲㸦㹀㸧:▼ᒣᬛ᫂㸦௦⾲⪅㸧㸪2013-2015 ᖺ㸪350 ୓(┤᥋⤒㈝)ࠕ㖟Ἑ⣔ෆࡢࢲ࣮ࢡ࣐ࢱ࣮ᚤ⣽ᵓ㐀ࡢゎ᫂࠾ࡼࡧࢲ࣮ࢡ࣐ࢱ᳨࣮ฟ࡬ࡢᛂ⏝ࠖ

50

ᖹᡂ 24 ᖺᗘ ⟃Ἴ኱Ꮫ ィ⟬⛉Ꮫ◊✲ࢭࣥࢱ࣮ ᖺḟሗ࿌᭩㸺ศᢸ⪅㸼࣭ᇶ┙◊✲㸦㸿㸧㸸ᱵᮧ㞞அ㸦ศᢸ⪅㸧㸦௦⾲⪅㸸኱ෆṇᕭ㸧 㸦2011 ᖺᗘ᥇ᢥ㸪⥅⥆㸧ࠕḟୡ௦኱つᶍ᥈ᰝ࡜ࢩ࣑࣮ࣗࣞࢩ࡛ࣙࣥᣮࡴᏱᐂ෌㟁㞳ࠖ (1 ୓෇)࣭ᇶ┙◊✲㸦㸿㸧㸸᳃ ṇኵ (ศᢸ⪅) 㸦௦⾲⪅㸸኱ෆṇᕭ㸧 㸦᪂つ㸧ࠕḟୡ௦኱つᶍ᥈ᰝ࡜ࢩ࣑࣮ࣗࣞࢩ࡛ࣙࣥᣮࡴᏱᐂ෌㟁㞳ࠖ (2.5 ୓෇)࣭ᇶ┙◊✲㸦㹁㸧㸸ᕝཱྀ ಇᏹ (ศᢸ⪅) 㸦௦⾲⪅㸸ᓠᓮ ᓅኵ㸧 㸦⥅⥆㸧ࠕάື㖟Ἑ᰾ከἼ㛗ࣔࢽࢱ࣮ࢹ࣮ࢱ࣮࣋ࢫ࡜άື㖟Ἑ᰾ኚග࣭ᨺᑕᶵᵓࡢ◊✲ࠖ(20୓෇)࣭ᣮᡓⓗⴌⱆ◊✲:ᕝ຾ ᮃ (ศᢸ⪅)㸦௦⾲⪅㸸㛗ᑿ㏱㸧㸦⥅⥆㸧Ᏹᐂࡢࠕ⏕ࡁࡓ໬▼ࠖ㸸ࠕ⌧ᅾࡢᏱᐂ࡟₯ࡴ㐍໬᭱ึᮇࡢ㖟Ἑ࡜ᕧ኱ࣈࣛࢵࢡ࣮࣍
ࣝࡢ᥈ᰝࠖ㸦15 ୓෇㸧

6.

◊✲ᴗ⦼
㸦㸯㸧◊✲ㄽᩥA) ᰝㄞ௜ࡁㄽᩥ
1) Doi, A., Nagira, H., Kawakatu, N. Kino, M., Nagai, H., Asada, K., 2012, Radio Galaxies
in Narrow-line Seyfert 1 Galaxies, The Astrophysical Journal, 760(1), 41-51
2) Godet, B. Plazolles, T. Kawaguchi, J.-P. Lasota, D. Barret, S. Farrell, V. Braito, M.
Servillat, N. Webb and N. Gehrels, 2012, Investigating slim disk solutions for HLX-1 in
ESO 243-49, The Astronomical Journal, 752, 34 [12pages]
3) Hasegawa, K., Semelin, B., 2013, The impacts of ultraviolet radiation feedback on
galaxies during the epoch of reionization, Monthly Notices of the Royal Astronomical
Society, Volume 428, pp.154-166
4) Ishiyama, T., Nitadori, K., Makino, J. 2012, 4.45 Pflops Astrophysical N-Body
Simulation on K computer – The Gravitational Trillion-Body Problem SC '12
Proceedings of the International Conference on High Performance Computing,
Networking, Storage and Analysis, Article No. 5
5) Kawata,D., Okamoto, T., Gibson, B. K., Barnes, D. J. and Cen, R., 2013, Calibrating an
updated smoothed particle hydrodynamics scheme within gcd+, Monthly Notices of theRoyal Astronomical Society, 428, 1968-1979
6) Kino, M., Kawakatu,N., Takahara, F., 2012, Calorimetry of AGN Jets: Testing Plasma
Composition in Cygnus A, The Astrophysical Journal, 751(2), 101-109

51

ᖹᡂ 24 ᖺᗘ ⟃Ἴ኱Ꮫ ィ⟬⛉Ꮫ◊✲ࢭࣥࢱ࣮ ᖺḟሗ࿌᭩7) Kino M., Ito, H., Kawakatu, N.,

Orienti, M., 2013, New class of very high energy -ray

emitter:radio-dark mini-shells surrounding in AGN jets, The Astrophysical Journal,764(2), 134-138
8) Komatsu, Y., Yamada, H., Kawamoto, S., Fukuda, M., Miyakawa, T., Morikawa, R.
Takasu, M., Akanuma, S. and Yamagishi, A., 2012, Designing the Binding Surface ofProteins to Construct Nano-fibers , Progress in Theoretical Chemistry and Physics--Quantum Systems in Chemistry and Physics, 26, 555-567
9) Komatsu, Y., Fukuda, M., Yamada, H., Kawamoto, S., Miyakawa, T., Morikawa, R.,
Takasu, M., Yokojima, S., Akanuma, S. and Yamagishi, A., 2012, Constructing Protein
Nano-Fiber and Estimation of the Electronic State Around Metal Ions, Int. J. Quantum
Chem., 112, 3750-3755
10) Matsuda, Y., Yamada, T., Hayashino, T., Yamauchi, R., Nakamura, Y., Morimoto, N.,
Ouchi, M., Ono, Y., Umemura, M., Mori, M., 2012, Diffuse Ly haloes around Lyemitters at z=3: do dark matter distributions determine the Ly spatial extents?,
Monthly Notices of the Royal Astronomical Society 425, 878-883.
11) Miki, Y., Takahashi, D., Mori,M.,2012, A Fast Implementation and Performance
Analysis of Collisionless N-body Code Based on GPGPU, Procedia Computer Science, 9,96-105㸦Proceeding of International Conference on Computational Science, ICCS 2012㸧
12) Nimori, M., Habe, A., Sorai, K., Watanabe, Y., Hirota, A., and Namekata, D., 2013,
Dense cloud formation and star formation in a barred galaxy, Monthly Notices of theRoyal Astronomical Society, 429, 2175-2182.
13) Okamoto, T., 2013, The origin of pseudo-bulges in cosmological simulations of galaxy
formation, Monthly Notices of the Royal Astronomical Society, 428, 718-728
14) Prokhorov, D. A., Million, E. T., Akahori, T., Zemcov, M., Moraghan, A., Nagataki, S.,
Yoshikawa, K., Colafrancesco, S., Rawle, T. D., Egami, E., 2012, A high-resolution studyof the X-ray emission and Sunyaev-Zel'dovich effect in the Bullet cluster (1E 0657-56),
Monthly Notices of the Royal Astronomical Society, 426, 2291-2299
15) Scannapieco, C., Wadepuhl, M., Parry, O. H., Navarro, J. F., Jenkins, A., Springel, V.,
Teyssier, R., Carlson, E., Couchman, H. M. P., Crain, R. A., Dalla Vecchia, C., Frenk, C.
S., Kobayashi, C., Monaco, P., Murante, G., Okamoto, T., Quinn, T., Schaye, J., Stinson,
G. S., Theuns, T., Wadsley, J., White, S. D. M.

and Woods, R., 2012, The Aquila

comparison project: the effects of feedback and numerical methods on simulations ofgalaxy formation, Monthly Notices of the Royal Astronomical Society, 423, 1726-1749

52

ᖹᡂ 24 ᖺᗘ ⟃Ἴ኱Ꮫ ィ⟬⛉Ꮫ◊✲ࢭࣥࢱ࣮ ᖺḟሗ࿌᭩16) Shimizu, I., Yoshida, N. and Okamoto, T., 2012, Submillimetre galaxies in cosmologicalhydrodynamic simulations: source number counts and the spatial clustering, Monthly
Notices of the Royal Astronomical Society, 427, 2866-2875
17) Son, D., Woo, J.H., Kim, S.C., Fu, H., Kawakatu, N., Bennert, V.N., Nagao, T., Park,D., 2012, Accretion Properties of High- and Low-Excitation Young Radio Galaxies, The
Astrophysical Journal, 757(2), 140-152
18) Tanikawa, A., Yoshikawa, K., Nitadori, K. and Okamoto, T., 2013, Phantom-GRAPE:
Numerical software library to accelerate collisionless N-body simulation with SIMD
instruction set on x86 architecture, New Astronomy, 19, 74-88
19) Umemura, M. Susa, H., Hasegawa, K., Suwa, T., Semelin, B., 2012, Formation andRadiative Feedback of First Objects and First Galaxies, Prog. Theor. Exp. Phys., 01A306(23pp)
20) Wagner, Y. , Bicknell, G. V. and Umemura, M. ,2012, Driving Outflows with Relativistic
Jets and the Dependence of Active Galactic Nucleus Feedback Efficiency on Interstellar
Medium Inhomogeneity, The Astronomical Journal, 757, 13621) Wagner, Y. , Umemura, M. and Bicknell, G. V. ,2013, Ultrafast Outflows: Galaxy-scale
Active Galactic Nucleus Feedback, The Astronomical Journal Letters, 763, L1822) Yajima, H., Umemura, M., Mori, M., 2012, Sub-millimetre brightness of earlystar-forming galaxies, Monthly Notices of the Royal Astronomical Society, 420,
3381-3388.
23) Yamada, K., Kitayama, T., Takakuwa, S., Iono, D., Tsutsumi, T., Kohno, K., Takizawa,
M., Yoshikawa, K., Akahori, T., Komatsu, E., Suto, Y., Matsuo, H., Kawabe, R., 2012,
Imaging Simulations of the Sunyaev-Zel'dovich Effect for ALMA, Publications of the
Astronomical, Society of Japan, 64, 10224) Yamada, T., Matsuda, Y., Kousai, K., Hayashino, T., Morimoto, N., Umemura, M., 2012,
Profiles of Lyman alpha Emission Lines, The Astronomical Journal, 751, 29-41.
25) Yamada, T., Nakamura, Y., Matsuda, Y., Hayashino, T., Yamauchi, R., Morimoto, N.,
Kousai, K., Umemura, M., 2012, Panoramic Survey of Ly Emitters at z = 3.1, The
Astronomical Journal, 143, 79-92.
26) Yamaoka, K., Allured, R. , Kaaret, P. , Kennea, J.A. , Kawaguchi, T. , Ghandi, P. ,Shaposhnikov, N. , Ueda, Y. , Nakahira, S. , Kotani, T. , Negoro, H. , Takahashi, I. ,Yoshida, A. and Kawai, N. , 2012, RXTE Follow-up Observations of the Black Hole53ᖹᡂ 24 ᖺᗘ ⟃Ἴ኱Ꮫ ィ⟬⛉Ꮫ◊✲ࢭࣥࢱ࣮ ᖺḟሗ࿌᭩Candidate MAXI J1659-152 Discovered by MAXI and Swift, Publications of the
Astronomical, Society of Japan, 64, 32 [15 pages]27) Yoshikawa, K., Yoshida, N., Umemura, M., 2013, Direct Integration of the CollisionlessBoltzmann Equation in Six-dimensional Phase Space: Self-gravitating Systems, The
Astrophysical Journal, 762, 11628) ᕝ຾ᮃ㸪ⓑᕝ཭⣖㸪ᮏከṇᑦ㸪ᡞ⏣ࡉࡺࡾ, ⟃Ἴ኱Ꮫ, 2012 ᖺ㸪⌮ᩘᏛ⏕ᛂ᥼ࣉࣟࢪ࢙ࢡࢺ
࡜ࢫ࣮ࣃ࣮ࢧ࢖࢚ࣥࢫࣁ࢖ࢫࢡ࣮ࣝ࡜ࡢ㛵ಀ, ኱Ꮫධヨ◊✲ࢪ࣮ࣕࢼࣝ, 23, pp185-190
29) ᡪ㇂㇦㸪୕ᮌὒᖹ㸪ᮔὈ♸㸪᳃ṇኵ㸪୰㔛┤ே㸪2013 ᖺ㸪㔜ຊከయ⣔⏝ Tree Code ࡢ୪ิGPU ໬࡟ࡼࡿィ⟬ຍ㏿㸪ࣁ࢖ࣃࣇ࢛࣮࣐ࣥࢫࢥࣥࣆ࣮ࣗࢸ࢕ࣥࢢ࡜ィ⟬⛉Ꮫࢩ࣏ࣥࢪ࣒࢘
ㄽᩥ㞟㸪Vol.2013㸪pp.146-155

B) ᰝㄞ↓ࡋㄽᩥ30) Hasegawa K. and Semelin, B., 2012, Impacts of Ultraviolet Radiation Feedback on the
Cosmic Reionization History, FIRST STARS IV -from Hayashi to the Future- AIP
Conference Proceedings, 1480, 267-27031) Ishiyama, T., Makino, J., Ebisuzaki, T., 2012, The formation and evolution of first dark
matter microhalos, FIRST STARS IV -from Hayashi to the Future- AIP Conference
Proceedings,, 1480, 382
32) Ogiya, G. and Mori, M., 2012, The Core-Cusp Problem in CDM Halos and Supernova
Feedback, Astronomical Society of the Pacific Conference Series, Vol. 458, pp. 385-387
33) Okamoto, T., 2012, Cosmological pseudobulge formation, 2012, FIRST STARS IV -fromHayashi to the Future- AIP Conference Proceedings, Volume 1480, 403-405
34) Shimizu I., Yoshida N., and Okamoto T., 2012, Lyman alpha emitters in cosmologicalsimulations: Lyman alpha escape fraction and statistical properties, FIRST STARS IV-from Hayashi to the Future- AIP Conference Proceedings, 1480, 412-414
35) Tanikawa, A., Yoshikawa, K., Nitadori,K. and Okamoto, T., 2012, Phantom-GRAPE:SIMD accelerated numerical library for N-body simulations, Astrophysics Source CodeLibrary, record ascl:1209.008
36) Tanikawa, A., and Umemura, M., 2011, Successive Merger of Multiple Massive Black
Holes in a Primordial Galaxy, FIRST STARS IV -from Hayashi to the Future- AIP
Conference Proceedings, 1480, 430-432
37) ᡪ㇂㇦㸪୕ᮌὒᖹ㸪ᮔὈ♸㸪᳃ṇኵ㸪୰㔛┤ே㸪2012 ᖺ㸪㔜ຊከయ⣔⏝ Tree Code ࡢ୪ิ54ᖹᡂ 24 ᖺᗘ ⟃Ἴ኱Ꮫ ィ⟬⛉Ꮫ◊✲ࢭࣥࢱ࣮ ᖺḟሗ࿌᭩GPU ໬㸪◊✲ሗ࿌ࣁ࢖ࣃࣇ࢛࣮࣐ࣥࢫࢥࣥࣆ࣮ࣗࢸ࢕ࣥࢢ㸦HPC㸧㸪2012-HPC-135 ᕳ㸪
40 ྕ㸪pp.1-938) ᡪ㇂㇦㸪᳃ṇኵ㸪2012 ᖺ㸪ᫍࣇ࢕࣮ࢻࣂࢵࢡ࡟ᑐࡍࡿ㖟Ἑ࢞ࢫࡢ᣺ࡿ⯙࠸ࡢゎᯒ㸸㖟Ἑᙧ≧࣭ᫍᙧᡂ⋡࡬ࡢ౫Ꮡᛶ㸪᪥ᮏὶయຊᏛ఍ ᖺ఍ 2012 ㅮ₇ㄽᩥ㞟㸪215 ྕ㸪pp.1-5(2) ᅜ㝿఍㆟Ⓨ⾲A) ᣍᚅㅮ₇
1) Okamoto, T., 2012, Shaping galaxies by feedback: satellites, discs, and bulges, Discgalaxy formation in a cosmological context, (May 14-18, 2012, Heidelberg,
Germany)
2) Tanikawa, A., 2012, Multiples in clusters ~ First binary formation via few-bodymodes~, (Aug.15 – 17, 2012, Kobe, Japan)
3) Wagner,A., Umemura,M., Bicknell,G., Hydrodynamic Simulations of AGN Jet and
UFO Feedback, (Oct.5, 2012, Nagoya, Japan)
4) Yoshikawa, K., 2012, An alternative to N-body methods in astrophysicalself-gravitating systems: Vlasov-Poisson simulations”, Conference on
Computational Physics (Oct. 14-18, 2012, Kobe, Japan)5) Yoshikawa, K., 2012, Vlasov-Poisson simulations of self-gravitating systems, The
5th East Asian Numerical Astrophysics Meeting (Oct. 29-Nov.2, 2012, Kyoto,
Japan)
6) Kawakatu, N., 2012, Dynamical evolution of AGN cocoons, Relativistic jets in AGNs
(Nov. 29, 2012, NAOJ, Japan)B) ୍⯡ㅮ₇1) Hasegawa, K., Semelin, B., Umemura, M., Impacts of Ultraviolet Radiation
Feedback on the Cosmic Reionization History, The Epoch of Reionization: Theory Simulations – Observations (Apr. 23-27, 2012, Strasbourg, France)2) Hasegawa, K., Semelin, B., Impacts of Ultraviolet Radiation Feedback on the
Cosmic Reionization History, FIRST STARS IV –from Hayashi to the Future- (May21-25, 2012, Kyoto, Japan)
3) Okamoto, T., Cosmological pseudobulge formation, FIRST STARS IV –from
Hayashi to the Future- (May 21-25, 2012, Kyoto, Japan)55

ᖹᡂ 24 ᖺᗘ ⟃Ἴ኱Ꮫ ィ⟬⛉Ꮫ◊✲ࢭࣥࢱ࣮ ᖺḟሗ࿌᭩4) Miki, Y., Takahashi, D., Mori, M., A Fast Implementation and Performance
Analysis of Collisionless N-body Code Based on GPGPU, International Conference
on Computational Science (Jun. 4-6, 2012, Omaha, USA)
5) Ogiya, G. and Mori, M., The Core-Cusp problem in Cold Dark Matter halos andSupernova feedback: Effects of Oscillation, IAP-Subaru Joint International
Conference: Stellar populations across Cosmic Times, (Jun. 25-29, 2012, Paris,
France)6) Kawakatu,N., Wada, K., 2012, Coevolution of AGNs and nuclear starbursts, AGN
Workshop 2012 in Jeju (Sep. 12㹼14, 2012, Jeju Island, Korea)
7) Kawaguchi, T. , Miki, Y. and Mori, M. , Emission from AGN Dusty Tori and a
Wandering BH, AGN Workshop 2012 in Jeju, (Sep. 12㹼14, 2012, Jeju Island,
Korea)
8) Wagner, A., Umemura, M., Bicknell, G., Mechanical Feedback by AGN Jets, First
East Asian AGN Workshop in Jeju, (Sep. 12-14, 2012, Jeju Island, Korea)
9) Ishiyama, T., Petascale Cosmological N-body Simulations, Conference on
Computational Physics (CCP2012), (Oct.14-18, 2012, Kobe, Japan)
10) Kirihara, T., Miki, Y., Mori, M., Resolving the outer density profile of dark matter
halo in Andromeda galaxy, Conference on Computational Physics(CCP2012),(Oct.14-18, 2012, Kobe, Japan)11) Miki, Y., Mori, M. and Kawaguchi, M., Hunting a Wandering Black Hole in M31
Halo Using GPU Cluster, Conference on Computational Physics 2012(CCP2012),(Oct.14-18, 2012, Kobe, Japan)12) Ogiya, G., Mori, M., Miki, Y., Boku, T. and Nakasato, N., Study of the core-cusp
problem in cold dark matter halos using N-body simulations on GPU clusters,
Conference on Computational Physics (CCP2012), (Oct.14-18, 2012, Kobe, Japan)
13) Ishiyama, T., The Gravitational Trillion-Body Problem on K computer, The
Fifth East Asian Numerical Astrophysics Meeting (EANAM 2012), (Oct. 29-Nov.2,
2012, Kyoto, Japan)
14) Kirihara, T., Miki, Y., Mori, M., Galaxy Collision and the Outer Density Profile inAndromeda Galaxy, East Asia Numerical Astrophysics Meeting(EANAM 2012),(Oct. 29-Nov. 2, 2012, Kyoto, Japan)15) Ogiya, G. and Mori, M., Landau resonance and the core-cusp problem in cold dark
matter halos, East Asia Numerical Astrophysics Meeting (EANAM2012),(Oct.29-Nov.2, 2012, Kyoto, Japan)56ᖹᡂ 24 ᖺᗘ ⟃Ἴ኱Ꮫ ィ⟬⛉Ꮫ◊✲ࢭࣥࢱ࣮ ᖺḟሗ࿌᭩16) Miki, Y., Mori, M., Kawaguchi, T., Galaxy Merger and Hungry Black Hole:Suppression of Black Hole Activity due to Galaxy Merger, East Asia Numerical
Astrophysics Meeting (EANAM2012), (Oct.29-Nov.2, 2012, Kyoto, Japan)17) Suzuki, H., Umemura, M., The impact of background and internal UV radiation on
the galaxy formation. , East Asia Numerical Astrophysics Meeting, 2012 Kyoto(EANAM 2012) , (Oct.29-Nov.2, 2012, Kyoto, Japan) (poster)18) Tanikawa A., 2012, Successive merger of multiple massive black holes in a
primordial galaxy and its effect on the galactic structure, (Oct. 29 – Nov. 2, 2012,
Kyoto, Japan)19) Kawaguchi, T. , Innermost Structure and Near-Infrared Emission of AGN Dusty
Tori, Torus Workshop 2012, U of Texas in San Antonio (Dec. 4-6,2012, USA),
20) Hasegawa, K., Okamoto, T., The improvement of START, Cosmological Radiative
Transfer Comparison Project Workshop IV (Dec. 12-14, 2012, Austin, USA,)21) Kawaguchi, T. , Growth of massive black holes revealed via the HSC survey,
Supermassive Black Holes in the Universe: The Era of the HSC Surveys, (Dec.18-20,
2012, Matsuyama ,Japan),22) Hasegawa, K., The improvement of a Radiation hydrodynamics code START, 3rd
AICS international Symposium, (Feb.28-Mar. 1, 2013, Kobe, Japan)(3) ᅜෆᏛ఍࣭◊✲఍Ⓨ⾲A) ᣍᚅㅮ₇1) ᒸᮏᓫ,ࠕ⌮ㄽࢩ࣑࣮ࣗࣞࢩ࡛ࣙࣥぢࡓ㖟Ἑᙧᡂ◊✲ࡢ⌧≧ (I) High-redshift discs andtheir descendants at z = 0ࠖ, 㖟Ἑᙧᡂゎ๗࣮࣡ࢡࢩࣙࢵࣉ "Resolved Views ofGalaxy Formation and Evolution", (2012 ᖺ 5 ᭶ 29 ᪥㹼31 ᪥, Hilo, Hawaii)2) ᱵᮧ㞞அ㸪ࠕ㖟Ἑ࣭AGN ᙧᡂ࡟㛵ࡍࡿ⌮ㄽⓗㄢ㢟ࠖ㸪◊✲఍ࠕࡍࡤࡿ HSC ࢧ࣮࣋࢖࡟
ࡼࡿࢧ࢖࢚ࣥࢫࠖ㸦2012 ᖺ 9 ᭶ 26 ᪥㹼28 ᪥㸪ᅜ❧ኳᩥྎ㸪୕㮚ᕷ㸧3) ▼ᒣᬛ᫂, ࠕࢫ࣮ࣃ࣮ࢥࣥࣆ࣮ࣗࢱ࣮ࡢ୰࡛⏕ࡲࢀࡿᏱᐂࠖ, ࢧ࢖࢚ࣥࢸ࢕ࣇ࢕ࢵࢡ࣭
ࢩࢫࢸ࣒◊✲఍ ⛉Ꮫᢏ⾡ィ⟬ศ⛉఍ 2012 ᖺᗘ఍ྜ(2012 ᖺ 10 ᭶ 24 ᪥, ANA ࢡࣛ࢘ࣥࣉࣛࢨ࣍ࢸࣝ⚄ᡞ)4) ୕ᮌὒᖹ, ࠕ࢞ࢫ㞼 G2 ⴠୗ࡟ࡼࡿ Sgr A*࡬ࡢ࢞ࢫ㝆╔ࠖ, ࠗ㖟Ἑ⣔୰ᚰࣈࣛࢵࢡ࣮࣍
ࣝ 2013࠘◊✲఍㸦2012 ᖺ 11 ᭶ 7 ᪥㹼9 ᪥, Ᏹᐂ⛉Ꮫ◊✲ᡤ, ┦ᶍཎᕷ㸧5) 㛗㇂ᕝ㈼஧㸪ࠕ኱つᶍ୪ิ໬࡬ྥࡅࡓ㍽ᑕ㍺㏦ࢥ࣮ࢻ START ࡢᨵⰋࠖ㸪➨ 25 ᅇ⌮ㄽ᠓ࢩ࣏ࣥࢪ࣒࢘, (2012 ᖺ 12 ᭶ 22 ᪥㹼24 ᪥㸪ࡘࡃࡤᅜ㝿఍㆟ሙ㸪ࡘࡃࡤᕷ)6) ▼ᒣᬛ᫂, ࠕࢲ࣮ࢡ࣐ࢱ࣮ࢩ࣑࣮ࣗࣞࢩࣙࣥࠖ, ➨ 25 ᅇ⌮ㄽ᠓ࢩ࣏ࣥࢪ࣒࢘, (2012 ᖺ
12 ᭶ 22 ᪥㹼24 ᪥㸪ࡘࡃࡤᅜ㝿఍㆟ሙ㸪ࡘࡃࡤᕷ)57

ᖹᡂ 24 ᖺᗘ ⟃Ἴ኱Ꮫ ィ⟬⛉Ꮫ◊✲ࢭࣥࢱ࣮ ᖺḟሗ࿌᭩7) ᕝ຾ᮃ㸪ࠕALMA ࡛᥈ࡿ㉸ᕧ኱ࣈࣛࢵࢡ࣮࣍ࣝᙧᡂࠖ
㸪ALMA ᫬௦ࡢᏱᐂᵓ㐀ᙧᡂ⌮ㄽ
㸦2013 ᖺ 1 ᭶ 25 ᪥㹼28 ᪥㸪໭ᾏ㐨኱Ꮫ㸪ᮐᖠᕷ㸧8) ᒸᮏᓫ, ࠕFormation of high-redshift disks and pseudo-bulges in nearby galaxiesࠖ,
ALMA ᫬௦ࡢᏱᐂࡢᵓ㐀ᙧᡂ⌮ㄽ㸸➨ 1 ୡ௦࠿ࡽ➨ n ୡ௦࡬ (2013 ᖺ 1 ᭶ 26 ᪥㹼
28 ᪥, ໭ᾏ㐨኱Ꮫ㸪ᮐᖠᕷ)9) ▼ᒣᬛ᫂, ࠕLarge scale dark matter simulationࠖ, ALMA ᫬௦ࡢᏱᐂࡢᵓ㐀ᙧᡂ⌮ㄽ㸸➨㸯ୡ௦࠿ࡽ➨㹬ୡ௦࡬(2013 ᖺ 1 ᭶ 26 ᪥㹼28 ᪥㸪໭ᾏ㐨኱Ꮫ㸪ᮐᖠᕷ)10) ▼ᒣᬛ᫂, ࠕ㉸୪ิ㔜ຊከయࢩ࣑࣮ࣗࣞࢩࣙࣥࢥ࣮ࢻࡢ㛤Ⓨࠖ, Ᏹᐂ☢Ẽὶయ࣭ࣉࣛࢬ࣐ࢩ࣑࣮ࣗࣞࢩ࣮ࣙࣥ࣡ࢡࢩࣙࢵࣉ(2013 ᖺ 2 ᭶ 18 ᪥㹼19 ᪥㸪༓ⴥ኱Ꮫ, ༓ⴥᕷ)11) ྜྷᕝ⪔ྖ, ࠕ↓⾪✺⮬ᕫ㔜ຊ⣔ࡢ↓⾪✺࣎ࣝࢶ࣐ࣥࢩ࣑࣮ࣗࣞࢩࣙࣥࠖ, Ᏹᐂ☢Ẽὶయ࣭ࣉࣛࢬ࣐ࢩ࣑࣮ࣗࣞࢩ࣮ࣙࣥ࣡ࢡࢩࣙࢵࣉ (2013 ᖺ 2 ᭶ 18 ᪥㹼19 ᪥, ༓ⴥ኱Ꮫ, ༓ⴥᕷ)12) ᕝ຾ᮃ㸪ࠕ㖟Ἑ࡜ࣈࣛࢵࢡ࣮࣍ࣝࡢඹ㐍໬ࠖ㸪㖟Ἑ㐍໬࡜㐲᪉Ᏹᐂ 2013㸦➨ 1 ᅇ㸧(2013ᖺ 2 ᭶ 20 ᪥㹼21 ᪥, ࢥ࣮ࣉ࢖ࣥி㒔, ி㒔ᕷ)13) ᕝ຾ᮃ㸪ࠕࢧࣈ࣑ࣜἼほ ࡛᥈ࡿάື㖟Ἑ᰾ࡢᙧᡂ࡜㐍໬ࠖ, ALMA ࣑ࣜἼࢧࣈ࣑ࣜἼ
ほ࡛ᢲࡉ࠼ࡿ㖟Ἑࡢᇶᮏほ㔞࡜ࡑࡢ⌮ゎ(2013 ᖺ 2 ᭶ 25 ᪥㹼26 ᪥, ᅜ❧ኳᩥྎ㸪୕㮚ᕷ)14) ᕝཱྀಇᏹ, ࠕ㟁Ἴほ ࡛᥈ࡿ㖟Ἑ⾪✺࡟క࠺ᕧ኱ࣈࣛࢵࢡ࣮࣍ࣝࡢᡂ㛗ࠖ, ࠕALMA ࣑ࣜἼࢧࣈ࣑ࣜἼほ࡛ᢲࡉ࠼ࡿ㖟Ἑࡢᇶᮏほ㔞࡜ࡑࡢ⌮ゎ࣮ࠖ࣡ࢡࢩࣙࢵࣉ(2013 ᖺ2 ᭶ 25 ᪥㹼26 ᪥, ᅜ❧ኳᩥྎ㸪୕㮚ᕷ)15) ᒸᮏᓫ, ࠕࢫ࣮ࣃ࣮ࢥࣥࣆ࣮ࣗࢱ࡟ࡼࡿ㖟Ἑᙧᡂࠖ, ➨㸷ᅇ ๰ᡂࢩ࣏ࣥࢪ࣒࢘, ࠕࢫ࣮ࣃ࣮ࢥࣥࣆ࣮ࣗࢱ "ி"࡛ࡏࡲࡿ᭱ඛ➃ࡢ⛉Ꮫ࣭ᢏ⾡ࠖ(2013 ᖺ 3 ᭶ 4 ᪥㸪໭ᾏ㐨኱Ꮫ㸪ᮐᖠᕷ)16) ▼ᒣᬛ᫂, ࠕࢫ࣮ࣃ࣮ࢥࣥࣆ࣮ࣗࢱࠕிࠖࡢ୰ࡢᏱᐂࠖ, 2012 ᖺᗘ HPCI ᡓ␎ࣉࣟࢢࣛ
࣒ศ㔝㸳඲యࢩ࣏ࣥࢪ࣒࢘㸦2013 ᖺ 3 ᭶ 5 ᪥㹼6 ᪥ 㸪ᐩኈࢯࣇࢺ࢔࢟ࣂࣉࣛࢨ㸧17) ᕝཱྀಇᏹ, ࠕᕧ኱ࣈࣛࢵࢡ࣮࣍ࣝࡢᙧᡂ࣭ᡂ㛗࡜㖟Ἑ࡜ࡢඹ㐍໬ࠖ, ᪥ᮏኳᩥᏛ఍᫓Ꮨ
ᖺ఍㸦2013 ᖺ 3 ᭶ 20 ᪥㹼23 ᪥, ᇸ⋢኱Ꮫ㸧B) ࡑࡢ௚ࡢⓎ⾲1) ᕝཱྀಇᏹ, ࠕάື㖟Ἑ᰾ࡢࢲࢫࢺࢺ࣮ࣛࢫ㸪ཬࡧ୰㛫㉁㔞ࣈࣛࢵࢡ࣮࣍ࣝࡢ᥈ᰝࠖ, ⌮ㄽ㒊ࣉࣛࢬ࣐ࢭ࣑ࢼ࣮㸦2012 ᖺ 5 ᭶ 18 ᪥, ᅜ❧ኳᩥྎ㸪୕㮚ᕷ㸧2) ᕝ຾ᮃ㸪 ⓑᕝ཭⣖㸪ᮏከṇᑦ㸪ᡞ⏣ࡉࡺࡾࠕ⟃Ἴ኱Ꮫࠕ⌮ᩘᏛ⏕ᛂ᥼ࣉࣟࢪ࢙ࢡࢺࠖ
࡜ࢫ࣮ࣃ࣮ࢧ࢖࢚ࣥࢫࣁ࢖ࢫࢡ࣮ࣝ࡜ࡢ㛵ಀࠖ,ࠗᖹᡂ 24 ᖺᗘ඲ᅜ኱ᏛධᏛ⪅㑅ᢤ◊✲㐃⤡༠㆟఍࠘ᒸᒣࢥࣥ࣋ࣥࢩࣙࣥࢭࣥࢱ࣮㸦2012 ᖺ 6 ᭶ 1 ᪥㸪ᒸᒣ㸪ᒸᒣᕷ㸧

58

ᖹᡂ 24 ᖺᗘ ⟃Ἴ኱Ꮫ ィ⟬⛉Ꮫ◊✲ࢭࣥࢱ࣮ ᖺḟሗ࿌᭩3) Wagner, A., Umemura, M. and Bicknell, G.,ࠕMechanical Feedback by AGN Jetsࠖ,Matsuyama Black Hole Workshop (2012 ᖺ 6 ᭶ 20 ᪥㹼23 ᪥, ឡ፾኱Ꮫ, ᯇᒣᕷ)4) ᕝ຾ᮃ㸪࿴⏣᱇୍㸪
ࠕAGN-Nuclear SB connection in Compton thick AGNࠖ,ᯇᒣࣈࣛࢵࢡ࣮࣮࣍ࣝ࣡ࢡࢩࣙࢵࣉ 2012ASTRO-H ⾨࡛ᫍ┠ᣦࡍࣈࣛࢵࢡ࣮࣍ࣝ◊✲ࡢ᪂ᒎ㛤㸦2012 ᖺ 6 ᭶ 23 ᪥㸪ឡ፾኱Ꮫ㸪ᯇᒣᕷ㸧5) ᕝཱྀಇᏹ, ࠕࢲࢫࢺࢺ࣮ࣛࢫࡢ᭱ෆ⦕ᵓ㐀ࣔࢹࣝࠖ, ASTRO-H ⾨࡛ᫍ┠ᣦࡍࣈࣛࢵࢡ
࣮࣍ࣝ◊✲ࡢ᪂ᒎ㛤 ◊✲఍㸦2012 ᖺ 6 ᭶ 22 ᪥㹼23 ᪥, ឡ፾኱Ꮫ㸧6) ᕝཱྀಇᏹ, ࠕ⁻࠺ᕧ኱ࣈࣛࢵࢡ࣮࣍ࣝ࡜୰㛫㉁㔞ࣈࣛࢵࢡ࣮࣍ࣝࡢ᥈ᰝࠖ, 㖟Ἑ୰ᚰ㉸ᕧ኱ࣈࣛࢵࢡ࣮࣍ࣝࡢ㉳※ ◊✲఍㸦2012 ᖺ 7 ᭶ 26㹼27 ᪥, ⟃Ἴ኱Ꮫ㸧7) 㕥ᮌ⿱⾜, ࠕ⣸እ⥺㍽ᑕሙ࡟࠾ࡅࡿཎጞ㖟Ἑᙧᡂࡢ≀⌮ࠖ,2012 ᖺᗘ➨ 42 ᅇኳᩥ࣭ኳ
య≀⌮ⱝᡭ ኟࡢᏛᰯ,(2012 ᖺ 8 ᭶ 3 ᪥ࠥ6 ᪥, ⚟஭┴ᮾᑜᆓ Ἠ୕ᅜほග࣍ࢸࣝ, ⚟஭┴) (ཱྀ㢌Ⓨ⾲)8) ୕ᮌὒᖹ, ᳃ṇኵ, ᕝཱྀಇᏹ, ࠕ㖟Ἑ⾪✺࡟ࡼࡿ㖟Ἑ୰ᚰᕧ኱ࣈࣛࢵࢡ࣮࣍ࣝ࿘㎶࠿ࡽࡢ࢞ࢫ๤ࡂྲྀࡾ㐣⛬ࠖ, VLBI WORKSHOPࠕᕧ኱ࣈࣛࢵࢡ࣮࣍ࣝ࠿ࡽࡢᄇฟὶࠖ㸦2012ᖺ 9 ᭶ 6 ᪥㹼7 ᪥, ᅜ❧ኳᩥྎ, ୕㮚ᕷ㸧9) ᡪ㇂㇦㸪᳃ṇኵ㸪ࠕᫍࣇ࢕࣮ࢻࣂࢵࢡ࡟ᑐࡍࡿ㖟Ἑ࢞ࢫࡢ᣺ࡿ⯙࠸ࡢゎᯒ㸸㖟Ἑᙧ≧࣭ᫍᙧᡂ⋡࡬ࡢ౫Ꮡᛶࠖ㸪᪥ᮏὶయຊᏛ఍ ᖺ఍ 2012㸦2012 ᖺ 9 ᭶ 16 ᪥㹼18 ᪥㸪㧗▱㸧10) ᳃ṇኵ㸪᪂⏣ఙஓ㸪஬༑ᔒᮒኟ㸪ࢥ࣮ࣝࢻࢲ࣮ࢡ࣐ࢱ࣮ࣁ࣮ࣟ࡟࠾ࡅࡿ㑄㡢㏿㖟Ἑ㢼ゎᯒ㸪᪥ᮏὶయຊᏛ఍ ᖺ఍ 2012㸦2012 ᖺ 9 ᭶ 16 ᪥㹼18 ᪥㸪㧗▱㸧11) ஬༑ᔒᮒኟ㸪᳃ṇኵ㸪᪂⏣ఙஓ㸪ࠕ⌫ᑐ⛠➼ᐃᖖ㖟Ἑ㢼ࡢຍ㏿㐣⛬࡟୚࠼ࡿࢲ࣮ࢡ࣐

ࢱ࣮࡜ᫍࡢ㉁㔞ศᕸࡢᙳ㡪ࠖ㸪᪥ᮏኳᩥᏛ఍⛅Ꮨᖺ఍(2012 ᖺ 9 ᭶ 19 ᪥㹼21 ᪥㸪኱ศ኱Ꮫ㸪኱ศᕷ)12) ▼ᒣᬛ᫂, ࠕி㏿ィ⟬ᶵ࡟ࡼࡿ↓⾪✺⣔㔜ຊከయࢩ࣑࣮ࣗࣞࢩࣙࣥࠖ, ᪥ᮏኳᩥᏛ఍⛅Ꮨᖺ఍㸦2012 ᖺ 9 ᭶ 19 ᪥㹼21 ᪥㸪኱ศ኱Ꮫ, ኱ศᕷ㸧13) ᑠஂಖ඘㸪ㅖ㝰ᬛ㈗㸪ᓠᓮᓅኵ㸪ᅵᒃᏲ㸪ྜྷ஭ㆡ㸪㉺⏣㐍ኴ㑻㸪ᕝཱྀಇᏹ㸪㩪ᓥᐶ᫂㸪ᑠᯘ⾜Ὀ,ࠕQSOs ࡢගᗘኚື࡟క࠺⣸እ࣮࢝ࣛኚື࡟ᑐࡍࡿᶆ‽෇┙+㉁㔞㝆╔⋡ኚ໬ࣔࢹࣝࡢጇᙜᛶࠖ,᪥ᮏኳᩥᏛ఍⛅Ꮨᖺ఍㸦2012 ᖺ 9 ᭶ 19 ᪥㹼21 ᪥㸪኱ศ኱Ꮫ, ኱ศᕷ㸧14) ᡪ㇂㇦㸪᳃ṇኵ㸪ࠕᫍࣇ࢕࣮ࢻࣂࢵࢡ࡟ᑐࡍࡿ㖟Ἑ࢞ࢫࡢ᣺ࡿ⯙࠸ࡢゎᯒ㸸㖟Ἑᙧ≧࣭ᫍᙧᡂ⋡࡬ࡢ౫Ꮡᛶࠖ㸪᪥ᮏኳᩥᏛ఍⛅Ꮨᖺ఍㸦2012 ᖺ 9 ᭶ 19 ᪥㹼21 ᪥㸪኱ศ኱Ꮫ, ኱ศᕷ㸧15) ᕝ຾ ᮃ㸪⣖ᇶᶞ㸪ࠕ⭾ᙇࢥࢡ࣮ࣥຊᏛ࠿ࡽ᥈ࡿ AGN ࢪ࢙ࢵࢺࡢࣉࣛࢬ࣐⤌ᡂ:㝧㟁Ꮚࡣᚲせ࠿㸽ࠖ㸪᪥ᮏኳᩥᏛ఍⛅Ꮨᖺ఍㸦2012 ᖺ 9 ᭶ 19 ᪥㹼21 ᪥㸪኱ศ኱Ꮫ, ኱ศᕷ㸧16) ᕝཱྀಇᏹ, O. Godet, B. Plazolles, ࠕᴟ㧗ගᗘ X ⥺※ࡢ 2 ୓ኴ㝧㉁㔞ࣈࣛࢵࢡ࣮࣍ࣝೃ
⿵ࠖ, ᪥ᮏኳᩥᏛ఍⛅Ꮨᖺ఍㸦2012 ᖺ 9 ᭶ 19 ᪥㹼21 ᪥㸪኱ศ኱Ꮫ, ኱ศᕷ㸧59

ᖹᡂ 24 ᖺᗘ ⟃Ἴ኱Ꮫ ィ⟬⛉Ꮫ◊✲ࢭࣥࢱ࣮ ᖺḟሗ࿌᭩17) ᱒ཎᓫர, ᳃ṇኵ, ࠕ࢔ࣥࢻ࣓ࣟࢲࢫࢺ࣮࣒ࣜࡢ㠀ᑐ⛠ᵓ㐀࡜ẕ▸ᑠ㖟Ἑࡢෆ㒊ᵓ㐀ࠖ,᪥ᮏኳᩥᏛ఍⛅Ꮨᖺ఍ 㸦2012 ᖺ 9 ᭶ 19 ᪥㹼21 ᪥㸪኱ศ኱Ꮫ, ኱ศᕷ㸧18) ୕ᮌὒᖹ, ᳃ṇኵ, ᕝཱྀಇᏹ, ⃽⸨♸⌮Ꮚ, ࠕM31 ࣁ࣮ࣟࢆ⁻࠺ᕧ኱ࣈࣛࢵࢡ࣮࣍ࣝ᥈
ᰝ: ⾪✺㖟Ἑࡢ✺ධ㌶㐨࡬ࡢไ㝈ࠖ, ᪥ᮏኳᩥᏛ఍⛅Ꮨᖺ఍, 㸦2012 ᖺ 9 ᭶ 19 ᪥㹼21᪥㸪኱ศ኱Ꮫ, ኱ศᕷ㸧19) ㇂ᕝ⾪, ᱵᮧ㞞அ㸪ࠕᕧ኱ࣈࣛࢵࢡ࣮࣍ࣝከయ⣔࡟࠾ࡅࡿࣈࣛࢵࢡ࣮࣍ࣝࡢ㐍໬࡜㖟Ἑࡢᵓ㐀ࠖ, ᪥ᮏኳᩥᏛ఍⛅Ꮨᖺ఍, 㸦2012 ᖺ 9 ᭶ 19 ᪥㹼21 ᪥㸪኱ศ኱Ꮫ, ኱ศᕷ㸧20) Wagner, A., Umemura, M. and Bicknell, G.ࠕMechanical Feedback by AGN Jets andUFOsࠖ,᪥ᮏኳᩥᏛ఍⛅Ꮨᖺ఍, 㸦2012 ᖺ 9 ᭶ 19 ᪥㹼21 ᪥㸪኱ศ኱Ꮫ, ኱ศᕷ㸧21) ୕ᮌὒᖹ, 㧗ᶫ኱௓, ᳃ṇኵ, ࠕ኱つᶍ GPU ࢡࣛࢫࢱ࡟࠾ࡅࡿ N యィ⟬ࢥ࣮ࢻࡢ₇⟬ᛶ⬟࡜ࢫࢣ࣮ࣛࣅࣜࢸ࢕ࡢホ౯ࠖ, ➨ 136 ᅇ ࣁ࢖ࣃࣇ࢛࣮࣐ࣥࢫࢥࣥࣆ࣮ࣗࢸ࢕ࣥ
ࢢ◊✲Ⓨ⾲఍, 㸦2012 ᖺ 10 ᭶ 3 ᪥㹼4 ᪥, Ἀ⦖⏘ᴗᨭ᥼ࢭࣥࢱ࣮, 㑣ぞᕷ㸧22) Wagner, A., Umemura, M. and Bicknell, G.ࠕHydrodynamic Simulations of AGN
Feedback in a Multiphase Mediumࠖ,ኳయᙧᡂ◊✲఍,(2012 ᖺ 10 ᭶ 5 ᭶㹼6 ᭶, ⟃Ἴ኱Ꮫ, ࡘࡃࡤᕷ)23) ᑠᯇຬ, ᱵᮧ㞞அ, ᗉྖග⏨, ▮ⰼ୍ᾈ, ⓑ▼㈼஧, ⚄㇂ඞᨻ, ᰰ἟ឡ, ⏣ཱྀ┿ᙪ, బ⸨ⓡඔ, ⸽ ᇆᡂ, ࠕ⣔እᝨᫍࡢࣂ࢖᳨࣐࣮࣮࢜࢝ฟ࡟ྥࡅࡓගྜᡂ࢔ࣥࢸࢼᶵᵓࡢບ㉳≧ែィ⟬ࠖ, ➨㸳ᅇ࢔ࢫࢺࣟࣂ࢖࢜ࣟࢪ࣮࣮࣡ࢡࢩࣙࢵࣉ㸦2012 ᖺ 11 ᭶, ᅜ❧ኳᩥྎ,୕㮚ᕷ㸧24) ⾜᪉኱㍜㸪ᱵᮧ㞞அ㸪㛗㇂ᕝ㈼஧㸪
ࠕAGN ࡢ㍽ᑕ࡟ࡉࡽࡉࢀࡓศᏊ㞼ࡢ㐍໬࡟ࡘ࠸࡚ࠖ
㸪
CfCA ࣮ࣘࢨ࣮ࢬ࣑࣮ࢸ࢕ࣥࢢ㸦2012 ᖺ 12 ᭶ 11 ᪥㹼12 ᪥㸪ᅜ❧ኳᩥྎ㸪୕㮚ᕷ㸧[࣏ࢫࢱ࣮Ⓨ⾲]
25) ୕ᮌὒᖹ, ᳃ṇኵ, ᕝཱྀಇᏹ, ࠕN యィ⟬࡟ࡼࡿ M31 ࣁ࣮ࣟ㡿ᇦࢆ⁻࠺ᕧ኱ࣈࣛࢵࢡ࣍
࣮ࣝ᥈ᰝࠖ, ➨ 25 ᅇ⌮ㄽ᠓ࢩ࣏ࣥࢪ࣒࢘ 㸦2012 ᭶ 12 ᪥ 22 ᪥㹼24 ᪥, ࡘࡃࡤᅜ㝿఍㆟ሙ, ࡘࡃࡤᕷ㸧26) ஬༑ᔒᮒኟ㸪᳃ṇኵ㸪᪂⏣ఙஓ㸪ࠕ⌫ᑐ⛠➼ᐃᖖ㖟Ἑ㢼ࡢ㑄㡢㏿ゎᯒࠖ㸪➨ 25 ᅇ⌮ㄽ᠓ࢩ࣏ࣥࢪ࣒࢘(2012 ᭶ 12 ᪥ 22 ᪥㹼24 ᪥, ࡘࡃࡤᅜ㝿఍㆟ሙ, ࡘࡃࡤᕷ)27) ᡪ㇂㇦㸪᳃ṇኵ㸪ࠕࣛࣥࢲ࢘ඹ㬆ࡀ୚࠼ࡿࢲ࣮ࢡ࣐ࢱ࣮ࣁ࣮ࣟᐦᗘᵓ㐀࡬ࡢᙳ㡪ࠖ㸪➨
25 ᅇ⌮ㄽ᠓ࢩ࣏ࣥࢪ࣒࢘ࠕィ⟬Ᏹᐂ≀⌮Ꮫࡢ᪂ᒎ㛤ࠖ(2012 ᭶ 12 ᪥ 22 ᪥㹼24 ᪥, ࡘࡃࡤᅜ㝿఍㆟ሙ, ࡘࡃࡤᕷ)28) ᱒ཎᓫர, ୕ᮌὒᖹ, ᳃ṇኵ, ࠕ࢔ࣥࢻ࣓ࣟࢲࢫࢺ࣮࣒࡛ࣜ᥈ࡿࢲ࣮ࢡ࣐ࢱ࣮ࣁ࣮ࣟࡢ
ෆ㒊ᵓ㐀ࠖ, ➨ 25 ᅇ⌮ㄽ᠓ࢩ࣏ࣥࢪ࣒࢘(2012 ᭶ 12 ᪥ 22 ᪥㹼24 ᪥, ࡘࡃࡤᅜ㝿఍㆟
ሙ, ࡘࡃࡤᕷ)29) ᕝཱྀಇᏹ, ⃽⸨♸⌮Ꮚ, ୕ᮌὒᖹ, ᳃ṇኵ,ࠕ㖟Ἑࣁ࣮ࣟ୰ࢆ⁻࠺ᕧ኱ࣈࣛࢵࢡ࣮࣍ࣝ࡬
ࡢ࢞ࢫ㝆╔࡜ࡑࡢᗈἼ㛗ᇦᨺᑕࠖ, ➨ 25 ᅇ⌮ㄽ᠓ࢩ࣏ࣥࢪ࣒࢘ࠕィ⟬Ᏹᐂ≀⌮Ꮫࡢ᪂60

ᖹᡂ 24 ᖺᗘ ⟃Ἴ኱Ꮫ ィ⟬⛉Ꮫ◊✲ࢭࣥࢱ࣮ ᖺḟሗ࿌᭩ᒎ㛤ࠖ(2012 ᭶ 12 ᪥ 22 ᪥㹼24 ᪥, ࡘࡃࡤᅜ㝿఍㆟ሙ, ࡘࡃࡤᕷ)30) 㕥ᮌ⿱⾜,ᱵᮧ㞞அ,ࠕ⫼ᬒ࠾ࡼࡧෆ㒊⣸እ⥺㍽ᑕ࡟ࡼࡿ㖟Ἑࡢᫍᙧᡂྐ࡬ࡢᙳ㡪ࠖ, ➨25 ᅇ⌮ㄽ᠓ࢩ࣏ࣥࢪ࣒࢘ࠕィ⟬Ᏹᐂ≀⌮Ꮫࡢ᪂ᒎ㛤ࠖ(2012 ᭶ 12 ᪥ 22 ᪥㹼24 ᪥, ࡘࡃࡤᕷᅜ㝿఍㆟ሙ, ࡘࡃࡤᕷ) (࣏ࢫࢱ࣮Ⓨ⾲)31) ⾜᪉኱㍜㸪ᱵᮧ㞞அ㸪㛗㇂ᕝ㈼஧㸪
ࠕAGN ࡢ㍽ᑕ࡟ࡉࡽࡉࢀࡓศᏊ㞼ࡢ㐍໬࡟ࡘ࠸࡚ࠖ
㸪➨ 25 ᅇ⌮ㄽ᠓ࢩ࣏ࣥࢪ࣒࢘(2012 ᭶ 12 ᪥ 22 ᪥㹼24 ᪥, ࡘࡃࡤᅜ㝿఍㆟ሙ, ࡘࡃࡤᕷ)32) ᕝཱྀಇᏹ, ࠕ㖟Ἑ୰ᚰ࡟㙠ᗙࡍࡿᕧ኱ࣈࣛࢵࢡ࣮࣍ࣝ࿘㎶ࡢᵓ㐀࡜㖟Ἑ⾪✺࡟క࠺ᕧ኱
ࣈࣛࢵࢡ࣮࣍ࣝࡢᡂ㛗ࠖ, ஑ᕞኳᩥࢭ࣑ࢼ࣮㸦2013 ᖺ 1 ᭶ 26 ᪥㸪஑ᕞ኱Ꮫ㸪⚟ᒸᕷ㸧33) 㕥ᮌ⿱⾜,ᱵᮧ㞞அ, ࠕThe effect of ultraviolet radiation on the SFH and galactic
morphologyࠖ, ALMA ᫬௦ࡢᏱᐂࡢᵓ㐀ᙧᡂ⌮ㄽ:➨ 1 ୡ௦࠿ࡽ➨ n ୡ௦࡬ ව 2012ᖺᗘึ௦࣭ᫍึ௦㖟Ἑ◊✲఍ (2013 ᖺ 1 ᭶ 26 ᪥㹼28 ᪥, ໭ᾏ㐨኱Ꮫ㸪ᮐᖠᕷ)

(࣏

ࢫࢱ࣮Ⓨ⾲)
34) ᕝཱྀಇᏹ, ࠕ㏿ᗘศゎ࢚ࢥ࣮࣐ࢵࣆࣥࢢ࡛᥈ࡿᕧ኱ࣈࣛࢵࢡ࣮࣍ࣝ࿘㎶ࡢ࢞ࢫὶฟධࠖ,ᒸᒣ 3.8m ᪂ᮃ㐲㙾࡟ࡼࡿࢧ࢖࢚ࣥࢫ࣭⿦⨨࣮࣡ࢡࢩࣙࢵࣉ(2013 ᖺ 3 ᭶ 12 ᪥㹼13 ᪥,ᅜ❧ኳᩥྎ㸪୕㮚ᕷ)35) ᑠᯇຬ, ᱵᮧ㞞அ, ᗉྖග⏨, ▮ⰼ୍ᾈ, ⓑ▼㈼஧, ⚄㇂ඞᨻ, ᰰ἟ឡ, ⏣ཱྀ┿ᙪ, బ⸨ⓡඔ, ⸽ ᇆᡂ, ࠕ⣔እᝨᫍࣂ࢖᳨࣐࣮࣮࢜࢝ฟࢆ┠ᣦࡋࡓගྜᡂᶵᵓࡢ࢚ࢿࣝࢠ࣮⛣ືィ⟬ࠖ, ᪥ᮏኳᩥᏛ఍᫓Ꮨᖺ఍㸦2013 ᖺ 3 ᭶ 20 ᪥㹼23 ᪥㸪ᇸ⋢኱Ꮫ, ࡉ࠸ࡓࡲᕷ㸧36) Ᏻ㒊∾ே㸪ᱵᮧ㞞அ㸪㛗㇂ᕝ㈼஧㸪ࠕ3 ḟඖ㍽ᑕὶయィ⟬࡟ࡼࡿ⣸እ⥺㍽ᑕሙ୰ࡢᫍᅋ
ᙧᡂ㐣⛬ࡢ◊✲ࠖ㸪᪥ᮏኳᩥᏛ఍᫓Ꮨᖺ఍㸦2013 ᖺ 3 ᭶ 20 ᪥㹼23 ᪥㸪ᇸ⋢኱Ꮫ㸪ࡉ࠸ࡓࡲᕷ㸧37) ஬༑ᔒᮒኟ㸪᳃ṇኵ㸪᪂⏣ఙஓ㸪ࠕᐃᖖ㖟Ἑ㢼࡟࠾ࡅࡿ㖟Ἑ୰ᚰࣈࣛࢵࢡ࣮࣍ࣝࡢᙳ㡪ࠖ㸪᪥ᮏኳᩥᏛ఍᫓Ꮨᖺ఍㸦2013 ᖺ 3 ᭶ 20 ᪥㹼23 ᪥㸪ᇸ⋢኱Ꮫ㸪ࡉ࠸ࡓࡲᕷ㸧(࣏ࢫࢱ࣮Ⓨ⾲㸪ᰝㄞ࠶ࡾ)38) ᑠ⏣ᐶ, ᕝཱྀಇᏹ, ࠕගᏛⓗ࡟ⷧ࠸☢Ẽᅽඃໃ෇┙࠿ࡽࡢᨺᑕࢫ࣌ࢡࢺࣝ: ᫂ࡿ࠸ࣁ࣮
ࢻ≧ែ࡬ࡢ㐺⏝ࠖ, ᪥ᮏኳᩥᏛ఍᫓Ꮨᖺ఍(2013 ᖺ 3 ᭶ 20 ᪥㹼23 ᪥, ᇸ⋢኱Ꮫ㸪ࡉ࠸ࡓࡲᕷ)39) ᕝཱྀಇᏹ, ࠕ㏿ᗘศゎ࢚ࢥ࣮࣐ࢵࣆࣥࢢ࡛᥈ࡿᕧ኱ࣈࣛࢵࢡ࣮࣍ࣝ࿘㎶ࡢ࢞ࢫὶฟධࠖ,ᒸᒣ 3.8m ᪂ᮃ㐲㙾࡟ࡼࡿࢧ࢖࢚ࣥࢫ࣭⿦⨨࣮࣡ࢡࢩࣙࢵࣉ(2013 ᖺ 3 ᭶ 12 ᪥㹼13 ᪥,ᅜ❧ኳᩥྎ, ୕㮚ᕷ)40) ᱒ཎᓫர, ୕ᮌὒᖹ, ᕝཱྀಇᏹ, ᳃ṇኵ, ࠕ࢔ࣥࢻ࣓ࣟࢲࢫࢺ࣮࣒ࣜࡢ㠀ᑐ⛠ᵓ㐀࡜ẕ▸ᑠ㖟Ἑෆ㒊ᵓ㐀ࡢ㛵ಀࠖ, ᪥ᮏኳᩥᏛ఍᫓Ꮨᖺ఍ (2013 ᖺ 3 ᭶ 20 ᪥㹼23 ᪥, ᇸ⋢኱Ꮫ, ࡉ࠸ࡓࡲᕷ)41) ῭⸨♸⌮Ꮚ, ㅖ㝰ᬛ㈗, ᕝཱྀಇᏹ, ௒すᫀಇ, ⨾⃰࿴㝧඾, ᓠᓮᓅኵ, ᕝ຾ᮃ, 㛗ᑿ㏱,
ᯇᒸ೺ኴ, ኱஭῵, ௒℩ె௓, ࠕz~3 ࡢ QSO ࡛᥈ࡿ㉸ᕧ኱ࣈࣛࢵࢡ࣮࣍ࣝ࡜ẕ㖟Ἑࡢ

61

ᖹᡂ 24 ᖺᗘ ⟃Ἴ኱Ꮫ ィ⟬⛉Ꮫ◊✲ࢭࣥࢱ࣮ ᖺḟሗ࿌᭩ඹ㐍໬ࠖ, ᪥ᮏኳᩥᏛ఍᫓Ꮨᖺ఍ (2013 ᖺ 3 ᭶ 20 ᪥㹼23 ᪥, ᇸ⋢኱Ꮫ, ࡉ࠸ࡓࡲᕷ)42) 㕥ᮌ⿱⾜㸪ᱵᮧ㞞அ㸪ࠕ⣸እ⥺㍽ᑕ࡟ࡼࡿ㖟Ἑࡢᫍᙧᡂྐ࣭㖟Ἑᙧែ࡬ࡢᙳ㡪ࠖ, ᪥ᮏኳᩥᏛ఍᫓Ꮨᖺ఍(2013 ᖺ 3 ᭶ 20 ᪥㹼23 ᪥, ᇸ⋢኱Ꮫ, ࡉ࠸ࡓࡲᕷ) (ཱྀ㢌Ⓨ⾲)43) ᅵᒃ᫂ᗈ㸪⛙࿴ᘯ㸪୰すᗣ୍㑻㸪Ἑ㔝Ꮥኴ㑻㸪ᑎᓥ㞝୍㸪ᕝཱྀಇᏹ㸪⛅ᒣ࿴ᚨ㸪⃝⏣బ⸨⪽Ꮚ㸪ᑿᓮᚸኵ, ࠕALMA cycle-0 ࡛ᤊ࠼ࡓࢯࣥࣈࣞࣟ㖟Ἑ(M104) ࡢ㉸ᕧ኱㉁㔞
ࣈࣛࢵࢡ࣮࣍ࣝ࿘㎶ 10 ࢩࣗࣂࣝࢶࢩࣝࢺ༙ᚄ௜㏆࠿ࡽࡢ㟁Ἴᨺᑕࠖ, ᪥ᮏኳᩥᏛ఍᫓
Ꮨᖺ఍(2013 ᖺ 3 ᭶ 20 ᪥㹼23 ᪥, ᇸ⋢኱Ꮫ, ࡉ࠸ࡓࡲᕷ)44) ⾜᪉኱㍜㸪ᱵᮧ㞞அ㸪㛗㇂ᕝ㈼஧㸪
ࠕAGN ࡢ㍽ᑕ࡟ࡉࡽࡉࢀࡓ࢞ࢫ㞼ࡢ㍽ᑕὶయィ⟬ࠖ㸪᪥ᮏኳᩥᏛ఍᫓Ꮨᖺ఍(2013 ᖺ 3 ᭶ 20 ᪥㹼23 ᪥, ᇸ⋢኱Ꮫ, ࡉ࠸ࡓࡲᕷ) (ཱྀ㢌Ⓨ⾲)45) ୕ᮌὒᖹ, ᳃ṇኵ, ᕝཱྀಇᏹ, ࠕ኱つᶍ GPU ࢡࣛࢫࢱࢆ⏝࠸࡚᥈ࡿ㉸ᕧ኱ࣈࣛࢵࢡ࣍
࣮ࣝᡂ㛗ࡢ⌧ሙࠖ, ᪥ᮏኳᩥᏛ఍᫓Ꮨᖺ఍ 㸦2013 ᖺ 3 ᭶ 20 ᪥㹼23 ᪥㸪ᇸ⋢኱Ꮫ, ࡉ࠸ࡓࡲᕷ㸧(4) ⴭ᭩㸪ゎㄝグ஦➼࣭▼ᒣᬛ᫂, ᒾἼࠕ⛉Ꮫࠖ 2013 ᖺ 4 ᭶ྕ, ୡ⏺᭱኱つᶍࡢࢲ࣮ࢡ࣐ࢱ࣮ࢩ࣑ࣗࣞ
࣮ࢩ
ࣙࣥ

7.

␗ศ㔝㛫㐃ᦠ࣭ᅜ㝿㐃ᦠ࣭ᅜ㝿άື➼࠙␗ศ㔝㛫㐃ᦠࠚ1) ᫍ㛫࢔࣑ࣀ㓟 L ᆺ㐣๫ࡢ◊✲㸦ᱵᮧ㸧Ᏹᐂ࣭⏕࿨࣭≀ᛶศ㔝㛫㐃ᦠ࡟ࡼࡾ㸪Ᏹᐂ✵㛫࡛෇೫ගἼ࠿ࡽ࢔࣑ࣀ㓟ࡢ㙾ീ␗ᛶయ㐣๫ࢆᘬࡁ㉳ࡇࡍ㐣⛬࡟ࡘ࠸࡚ࡢ㔞Ꮚከయィ⟬ࢆ㐍ࡵࡓࠋ2) ⣔እᝨᫍ࡟࠾ࡅࡿගྜᡂ࢔ࣥࢸࢼᶵᵓࡢ◊✲㸦ᑠᯇ㸪ᱵᮧ㸧Ᏹᐂ࣭⏕࿨ศ㔝㛫㐃ᦠ࡟ࡼࡾ㸪⣔እᝨᫍ⣔ࡢ୺ᫍගࢫ࣌ࢡࢺࣝ࡜ගྜᡂගᤕ㞟ࡢ┦㛵ࢆᑟฟࡍࡿࡇ࡜ࢆ┠ⓗ࡟㸪㔞Ꮚ໬Ꮫィ⟬ࢆ㐍ࡵࡓࠋ࠙ᅜ㝿㐃ᦠࠚ
࣭Alex Wagner,
1) Collaboration with Prof. Joseph Silk (IAP, France) on the specific topic of "StarFormation in AGN-pressure confined Disk Galaxies."2) Collaboration with Dr. Kalliopi Dasyra, Prof. Francoise Combes, Dr. Greg Novak, Dr.
Julia Scharwaechter (Observatoire de Paris, France) on "Kpc-scale multiphase
outflows from AGN"

62

ᖹᡂ 24 ᖺᗘ ⟃Ἴ኱Ꮫ ィ⟬⛉Ꮫ◊✲ࢭࣥࢱ࣮ ᖺḟሗ࿌᭩ࢩ࣏ࣥࢪ࣒࢘㸪◊✲఍㸪ࢫࢡ࣮ࣝ➼ࡢ㛤ദᐇ⦼8.

1) ᅜ㝿఍㆟ࠕFIRST STARS IV - From Hayashi to the Future -ࠖ, May 22- 25, 2012㸪
Heartpia Kyoto, Kyoto, Japan2) ࣮࣡ࢡࢩࣙࢵࣉࠕᕧ኱ࣈࣛࢵࢡ࣮࣍ࣝࡢ㉳※ࠖ
㸪2012 ᖺ 7 ᭶ 26 ᪥㹼28 ᪥⟃Ἴ኱Ꮫィ⟬⛉Ꮫ◊✲ࢭࣥࢱ࣮㸪ࡘࡃࡤᕷ3) ◊✲఍ࠕAGN Workshop 2012 in Jejuࠖ㸪2012 ᖺ 9 ᭶ 12 ᪥㹼14 ᪥
http://astro.snu.ac.kr/~hjbae/Welcome.html
4) ࠕኳయᙧᡂ◊✲఍ࠖ2012 ᖺ 10 ᭶ 5 ᪥㹼6 ᪥⟃Ἴ኱Ꮫィ⟬⛉Ꮫ◊✲ࢭࣥࢱ࣮㸪ࡘࡃࡤᕷ5) ➨ 25 ᅇ⌮ㄽ᠓ࢩ࣏ࣥࢪ࣒࢘ࠕィ⟬Ᏹᐂ≀⌮Ꮫࡢ᪂ᒎ㛤ࠖ㸪2012 ᖺ 12 ᭶ 22 ᪥㸦ᅵ㸧㸫 24᪥㸦᭶㸧㸪ࡘࡃࡤᅜ㝿఍㆟ሙ, ࡘࡃࡤᕷ⟶⌮࣭㐠Ⴀ㸦⤌⧊㐠Ⴀࡸᨭ᥼ᴗົࡢጤဨ࣭ᙺဨࡢᐇ⦼㸧

9.

࣭ᱵᮧ㞞அ
ィ⟬⛉Ꮫ◊✲ࢭࣥࢱ࣮ 㐠Ⴀጤဨ఍ጤဨ
ィ⟬⛉Ꮫ◊✲ࢭࣥࢱ࣮ ๪ࢭࣥࢱ࣮㛗ィ⟬⛉Ꮫ◊✲ࢭࣥࢱ࣮ ඹྠ฼⏝ጤဨ఍୺ᰝ
ィ⟬⛉Ꮫ◊✲ࢭࣥࢱ࣮ ඹྠ฼⏝ᑂᰝጤဨ఍ጤဨ㛗ィ⟬⛉Ꮫ◊✲ࢭࣥࢱ࣮ Ᏹᐂ࣭ཎᏊ᰾≀⌮◊✲㒊㛛୺௵ィ⟬⛉Ꮫ◊✲ࢭࣥࢱ࣮ 㐠Ⴀ༠㆟఍ጤဨィ⟬⛉Ꮫ◊✲ࢭࣥࢱ࣮ ◊✲௻⏬ᐊጤဨ≀⌮Ꮫᇦ 㐠Ⴀጤဨ఍ጤဨ
≀⌮Ꮫᇦ Ᏹᐂ≀⌮⌮ㄽࢢ࣮ࣝࣉ㛗≀⌮Ꮫ㢮 ࣒࢝ࣜ࢟ࣗࣛጤဨ఍ጤဨ㛗㸪Ꮫົጤဨ࣭ྜྷᕝ⪔ྖィ⟬⛉Ꮫ◊✲ࢭࣥࢱ࣮࣭ࣇࣟࣥࢸ࢕࢔ィ⟬ᶵࢩࢫࢸ࣒௙ᵝ⟇ᐃጤဨ఍࣭ጤဨ㸦᭩グ㸧ィ⟬⛉Ꮫ◊✲ࢭࣥࢱ࣮࣭ᐦ⤖ྜ୪ิ₇⟬ຍ㏿ᶵᵓᐇ㦂ࢩࢫࢸ࣒௙ᵝ⟇ᐃጤဨ఍࣭ጤ
ဨ
10. ♫఍㈉⊩࣭ᅜ㝿㈉⊩63ᖹᡂ 24 ᖺᗘ ⟃Ἴ኱Ꮫ ィ⟬⛉Ꮫ◊✲ࢭࣥࢱ࣮ ᖺḟሗ࿌᭩࣭ᕝ຾ᮃ1) ኱Ꮫㄝ᫂఍࣭ᶍᨃᤵᴗ㸦༓ⴥ┴❧బ಴㧗➼Ꮫᰯ㸧, 2012 ᖺ 5 ᭶ 8 ᪥,2) ᖹᡂ 24 ᖺᗘ⟃Ἴ኱Ꮫㄝ᫂఍, 2012 ᖺ 7 ᭶ 31 ᪥㸪⟃Ἴ኱Ꮫࠕ㖟Ἑ୰ᚰ࡟₯ࡴ㉸ᕧ኱ࣈࣛࢵࢡ࣮࣍ࣝᙧᡂࡢㅦࠖ
3) SSH ⏕ᚐ◊✲Ⓨ⾲఍ 2012 (ࣃࢩࣇ࢕ࢥᶓ὾㸪ᶓ὾ᕷ), 2012 ᖺ 8 ᭶ 8 ᪥㹼9 ᪥ 㸪⌮ᩘᏛ⏕ᛂ᥼ࣉࣟࢪ࢙ࢡࢺᗈሗ
4) ᮾி኱Ꮫ୺ദ୺せ኱Ꮫㄝ᫂఍㸦኱⏣༊⏘ᴗ㺪㺽㺵㺙㺼 PiO㸪ᮾி㸧,2012 ᖺ 8 ᭶ 21 ᪥⌮ᩘᏛ⏕ᛂ᥼ࣉࣟࢪ࢙ࢡࢺㄝ᫂
࣭ᕝཱྀಇᏹ1)ࠕࣈࣛࢵࢡ࣮࣍ࣝࡔࡽࡅࡢᏱᐂࠖ, ඲ᅜྠ᫬୐ኤㅮ₇఍ 2012 (2012 ᖺ 7 ᭶ 14 ᪥,ࡘࡃࡤᅜ㝿఍㆟ሙ, ࡘࡃࡤᕷ)11. ࡑࡢ௚㸦ᾏእ㛗ᮇ⁫ᅾ㸪ࣇ࢕࣮ࣝࢻ࣮࣡ࢡ࡞࡝㸧࡞ࡋ

64