NOBE YAMA RADIO OBSE RVAT ORY 2017.12- 2018.11 Ke n T a te ma - PowerPoint PPT Presentation

NOBE YAMA RADIO OBSE RVAT ORY 2017.12- 2018.11 Ke n T a te ma tsu, Dire c tor

SUMMARY • Numb e r o f sta ff me mb e rs 職員数 =39 (2 me mb e rs in Mita ka )  to b e <15 in 2022 Apr • Numb e r o f ye a rly re fe re e d pa pe rs 論文数 =30 (45m), 4 (So la r No RP, b ut 3 a re supple me nta l use to X-ra y pa pe rs) • Ac hie ve d my 30- ye a rly- pa pe r promise for 45m (b ut I c a n pro mise o nly 15 ye a rly pa pe rs fo r re d uc e d b ud g e t/ ma npo we r Ope n Use 2019-2022) • 14 pa pe rs using 1MUS$ （運用予算 1 億円で 14 論文）

45M L E GACY PROJE CT S (2014-2017) ~ 1000 HR E ACH; F I T S DAT A RE L E ASE D (2018/ 6/ 1); S … レガシー累積論文数 CUMUL AT I VEPAPE R NUMBE R I • F UGIN (PI =Ume mo to ) 11 pa pe rs : Pub lishe d =8 (Ya ma g ishi+, Ume mo to +, Nishimura +, K o hno +,T o rii+X2,K uriki+,So fue +); Ac c e pte d =1 (F ujita +); Sub mitte d =2 (T o rii+, F ujita +) • COMING (PI =So ra i) 6 pa pe rs : Pub lishe d =2 (Mura o ka +, Ha ta ke ya ma +); Sub mitte d =4 (Ya jima +, Sa la k+, Mura o ka +, So ra i+) • Sta r F orma tion (PI =Na ka mura ) 8 pa pe rs : Pub lishe d =5 (Shimo ikura +, Do b a shi+, Na ka mura +, F e d d e rse n+, K o ng +); Sub mitte d =4 (Na ka mura +, I shii+, T a na b e +, K usune +) • AL L : T ota l=26 pa pe rs; Publishe d=15; Ac c e pte d=1; 26 レガシー論文 Submitte d=10 • PASJ Spe c ia l Issue (c oming soon) T ota l=17 pa pe rs; Ac c e pte d=7; Submitte d=10

ON 論文引用 10 年で 100 回引用の実績 CI T AT I • Na rio K uno +2007: 116 c ita tio ns (o ld L e g a c y) • Sa c hiko Ono d e ra +2010: 97 c ita tio ns (o ld L e g a c y) • Jin K o d a +2009: 111 c ita tio ns (CARMA+45 m) UGIN 論文 年 10 回以上引用のペース F • T o mo fumi Ume mo to +2017Oc t: 15 c ita tio ns in 14 mo nths • Atsushi Nishimura +2018Ma y: 13 c ita tio ns in 7 mo nths • Mikio K o hno +2018Ma y: 14 c ita tio ns in 7 mo nths

CT ASPE ONAL I DUCAT E

SCI E NT I F I C HI GHL I GHT S: CL OUD COL L I SI ON サイエンスのハイライト：分子雲の衝突 (5 PAPE RS) • F ukui+, K o hno +, Nishimura +, T o rii+, T o rii+

SCI E NT I F I C HI GHL I GHT S: SNR-CL OUD I NT E RACT I ON 超新星残骸と分子雲の相互作用 (2 PAPE RS) • Do b a shi+, K uriki+

SCI E NT I F I C HI GHL I GHT S: SUPPRE SSE D SF I N BAR 銀河のバーでの抑圧された星形成の原因 (2 PAPE RS) • E g usa +, Ma e d a +

S シェルの発見 SCI E NT I F I C HI GHL I GHT S: SHE L L (2 PAPE RS) • F e d d e rse n+, T sujimo to +

SCI E NT I F I C HI GHL I GHT S: F I L AME NT S 分子雲フィラメント (2 PAPE RS) • Arzo uma nia n+ (fo rma tio n), Sa a ja sto + (ma ss a c c re tio n)

NOBE YAMA-PL ANCK PROJE CT RE PORT OF A L ARGE PROGRAM a te ma tsu , Gwa nje o ng K im (No b e ya ma NAOJ) Ke n T As PI of the la rg e prog ra m, ra the r tha n Dire c tor

CHEMICAL EVOLUTION N2D+/ N2H+ OR DNC/ HNC IN COLD COLD CORES. DEUTERIUM FRATION D/ H . ION ORMAT <100 yr for N2D+/ N2H+ IO ~10 4- 5 yr for DNC/ HNC D/ H RAT OF (T Sa ka i+12) T AR F ONSE ST T IME ST ARL E SS ST AR- F ORMING

NOBE YAMA L ARGE PROGRAM (350 HR OVE R 2 YE ARS—2017 DE C T O 2019 MAY) • Co ld (10-20K ) c lumps fro m Pla nc k a ll- sky surve y (5’ re so lutio n)  JCMT SCUBA- 2 ima g ing (20” re so lutio n)  Nobe ya ma 45m 100GHz a nd 70GHz to wa rd ~SCUBA-2 c o re s • 1 st ye a r ha s finishe d , a nd 2 nd ye a r o b se rva tio n ha s just sta rte d (2018-12-8) • 126 Orio n c o re s + 97 c o re s in va rio us e nviro nme nts inc lud ing hig h N • 70 GHz sing le - pointing (N 2 D + , DNC, HN 13 C, c -C 3 H 2 ) a nd 100 GHz F ORE ST OT F ma pping (N 2 H + , HC 3 N, two CCS line s) • All 70- GHz sing le - pointing s a t 70 GHz towa rd 223 c ore s ha ve be e n c omple te d • In the proc e ss of 100- GHz OT F ma pping

NOBE YAMA-PL ANCK (PI =T AT E MAT SU ) AL MA F OL L OW- UP • AL MA suc c e ssful proposa ls ba se d on Nobe ya ma - Pla nc k L a rg e / pilot obse rva tion • 2016.2.00058.S: Physic a l a nd c he mic a l prope rtie s of c old Orion c ore s ve ry c lose to the onse t of sta r forma tion (PI: Ke n T a te ma tsu) • 2017.1.00707.S: Unve iling the na ture of the ve ry- low luminosity sourc e in the Pla nc k c old c lump G204NE (PI: Na omi Hira no) • 2018.1.00302.S: F ra g me nta tion a nd substruc ture s of de nse c ore s c lose to the onse t of sta r forma tion in the Orion c omple x (PI: T ie L iu) • AL MA suc c e ssful proposa ls re la te d to Nobe ya ma - Pla nc k • 2017.1.01320.S: On the prope rtie s of Cla ss 0/ I protoste lla r c ore s in the L a mbda Orionis mole c ula r c omple x (PI: Ke e - T a e Kim)

WE PL AN T O PUBL I SH AT T E N PAPE RS L E AST • I nitia l pa pe rs (in pre pa ra tion) • Gwa nje o ng K im+: 70 GHz sing le -po inting c a ta lo g o f d e ute rium fra c tio n • Gwa nje o ng K im+: Clo ud d yna mic s in fila me nta ry c lo ud s in Orio n • K e n T a te ma tsu+: ACA 7m fo llo w-up a nd so me No b e ya ma N2H+ ma ps • 2 nd sta g e • T ie L iu+: Re g io na l stud y o f G6.4 • T ie L iu+: Re g io na l stud y o f G35 • He e -We o n Yim+: Co mpa riso n b e twe e n sta rle ss a nd sta r-fo rming c o re s • He e -We o n Yim+: Co mpa riso n a mo ng Orio n A, B, a nd λ • Gwa nje o ng K im+: Ma pping o b se rva tio ns o f hig h d e ute rium d e nse c o re s • Gwa nje o ng K im+: I nve stig a tio n o f sub struc ture s in hig h d e ute rium PGCC c o re s with AL MA a nd No b e ya ma • K e n T a te ma tsu+: Co re ro ta tio n a nd spe c ific a ng ula r mo me ntum in va rio us e nviro nme nts • Na o mi Hira no +: Co mpa riso n with ma ssive sta r fo rma tio n the o rie s, in pa rtic ula r ma ssive sta r fo rma tio n the o rie s + a nd N 2 D + hype rfine struc ture • Sa to shi Oha shi+: Physic a l na ture o f c o re s thro ug h N 2 H fitting