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W4 West(AFGL 333) 領域におけるアンモニア分子輝線観測. 副島隆史 ( 大分大学 M2) 仲野誠(大分大学) 面高俊宏 , 半田利弘 , 亀﨑達也 , Ross Burns, 馬場達也 , 松尾光洋 , 宮崎竜之介 , 吉田友哉(鹿児島大学) 永山匠 , 砂田和良 , James Chibueze , 久野成夫( NAOJ ). 31th NRO Users Meeting (2013). Introduction. W3 Main. W4. - PowerPoint PPT Presentation
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W4 West(AFGL 333) 領域におけるアンモニア分子輝線観測副島隆史 ( 大分大学 M2)
仲野誠(大分大学)面高俊宏 , 半田利弘 , 亀﨑達也 , Ross Burns, 馬場達也 , 松尾光洋 , 宮崎竜之介 , 吉田友哉(鹿児島大学)永山匠 , 砂田和良 , James Chibueze, 久野成夫( NAOJ )31th NRO Users Meeting (2013)
Introduction
• Interaction HII region with molecular cloud
• W3/W4 HII region - High density layer
- - W3Main, W3(OH), AFGL333
• AFGL333-Ridge (Rivera-Ingraham et al. 2013) - 2.0 kpc (Xu et al. 2006) - chemical properties of massive
clumps (Sakai et al. 2007)
W4
AFGL333-Ridge
W3(OH)
W3 Main
Fig.1. Optical image by Roger Rao
Fig.2. IR image by Spitzer IRAC
W3
Instruments• NRO 45m telescope• H22 + SAM45 Period• 2013/1/26 – 2013/6/11 (total ~ 135 h) Lines• NH3(J,K) = (1,1), (2,2), (3,3) and H2O maser - velocity resolution ~ 0.38 km/s - HPBW ~ 73’’ Method• 1grid=37.5”×37.5”, total 267 positions
• NewStar – Noise level Trms ~ 0.043 K
Observations – Backup program
NH3
• Main cloud - 11.8’×6.2’ (6.9×3.6 pc) - dent in the east• BRC (SFO 05) - northeast
H2O• 2 H2O masers - one is newly detected
Results
dent
BRCmaser
Fig.3. NH3(1,1) Integrated intensity map
(K k
m/s
)
preliminary
(K k
m/s
)
Fig.5. The black eclipse shows the extent obtained N(NH3)
• τ = 0.63 ± 0.14• Trot = 16.1 ± 0.4 [K]
• N(NH3) = 1.55×1015 [cm-2]
• R = 0.9×2.9 [pc]• MLTE = 2600 M ,☉ Mvir = 1800 M☉
Fig.4. observed spectra in the NH3
Ta(K)
(km/s)
Results
preliminarypreliminary
• Broad velocity width - east• High temperature - north, east
Results
Fig.7. Rotational temperature map Fig.6. Velocity width map
30
28
26
24
22
20
18
16
14
(K)
2.5
1.5
1.0
3.0
2.0
(km
/s)
preliminary
preliminary
Discussion Broad velocity width and high Trot in the east
• IRAS 02245+6115 - B0.5 star - compact HII region (Hughes & Viner 1982)
• 2 clusters- IRAS 02245+6115- IRAS 02244+6117
Fig.8. IR image of the AFGL333-Ridge (left). The green contour shows the extent of the compact HII region (right).
IRAS 02244+6117
IRAS 02245+6115
b (d
egre
e)
1.4GHz (CGPS)
preliminary
b (d
egre
e)
l (degree)
• Broad velocity width and high Trot and in the east would be originated with compact HII region.
Fig.9. The relation of HII region to velocity-width
Fig.10. The relation of HII region to Trot
2.5
1.5
1.0
3.0
2.0
(km
/s)
Discussion Broad velocity width and high Trot in the east
Clusterposition
Centerposition
preliminary
preliminary