h 3 + : a new probe of the galactic center takeshi oka department of astronomy and astrophysics and...
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H3+: A new probe of the Galactic center
Takeshi Oka
Department of Astronomy and Astrophysicsand Department of Chemistry,
The Enrico Fermi Institute, The University of Chicago
ACS symposium “Molecules in Space”, Atlanta, March 30, 2006
Hot and diffuse clouds near the Galactic center probed by metastable H3
+
T. Oka, T. R. Geballe, M. Goto, T. Usuda, B. J. McCall, ApJ 632, 882 (2005)
6
5
4
3
2
1
0
H3+
Col
umn
Den
sity
(10
14cm
-2)
50403020100
E(B-V) (mag)
AFGL2136
W33A
MonR2 IRS 3
AFGL961E
AFGL490
AFGL2591
8
6
4
2
0
H3+
Col
umn
Den
sity
(10
14cm
-2)
6543210
E(B-V) (mag)
OphP Cygni
HD 183143
WR 118
Cyg OB2 12
WR 104
Cyg OB2 5
WR 121
HD 168607
HD 194279
GC IRS 3
2 Ori
HD 20041
Dense clouds
McCall, Geballe, HinkleOka, ApJ 522,338(1999)
Diffuse clouds
McCall, Hinkle, Geballe, Moriarty-Schieven, Evans,Kawaguchi, Takano, Smith, Oka, ApJ 567, 391 (2002)
Per
N(H3+) ~ 3.6 ×1012 cm-2 AV
N(H3+) ~ 4.4 ×1013 cm-2 AV
The ubiquitous H3+
Dense
Diffuse
n
100
1
L
1
10
AV
10
1
N(H3+)
1
1
X(H3+)
1
10
ζ
1
10
X(H3+)diffuse ~ 10 X(H3
+)dense
10-9
10-8
10-7
10-6
10-5
10-4
10-3
10-2
10-1
100
101
102
103
104
105
106
n(X
)
10-1
100
101
102
103
104
105
106
n(H)
Dense Clouds Diffuse Clouds
H2
HCO
C+H3
+
V
1
1000
(H3+)total
1
100
H3+ is a powerful probe for diffuse cloudsN(H2)
S
1
100
Sightlines toward the Galactic center
Mezger, Duschl, Zylka (1996)Georgelin, Georgelin (1976)
AV = 25 ~ 40
Cotera, Simpson, Erickson, Colgan,Burton, Allen, ApJS 192, 123 (2000)
Toward Sgr A*
AV ~ 30 [AV]DISM ~ 20 , [AV]MC ~ 10
Whittet, Boogert, Gerakines, Schutte,Tielens, de Graauw, Prusti, van Dishoeck,Wesselius, Wright, ApJ 490, 729 (1997)
N(H3+)DISM: N(H3
+)MC ~ 20 : 1
The Central Molecular Zone (CMZ)R ~ 200 pcM ~ 5 ×107 M⊙
Dominantly molecularn(H2) > 104 cm-3
Volume filling factor 0.110 % of total ISMHot gasHigh velocity dispersionLow dust temperature
Mezger, Duschl, Zylka, A&A Rev. (1996)
Morris, Serabyn, ARA&A (1996)
Genzel, Hollenbach, Townes (1994)
CMZ
OH, H2CO, CO, CS, NH3, HCN H3+
Yusef-Zadeh, Morris, AJ (1987)
Nagata et al. (1990)Okuda et al. (1990)
Extraordinary radio emission
The Quituplet
LaRosa, Kassim, Lazio, Hyman, AJ 119, 207 (2000)
H3+ in the (3, 3) metastable level
Goto, McCall, Geballe, Usuda,Kobayashi, Terada, OkaPASJ, 54, 951 (2002)
The Subaru Telescope
32.9 K
361 K
J
KV = 2← 0
J
K
361 K
(J, K)
The ideal energy levels of H3+
(3, 3) metastable level
(1, 1) ground level
Δk = ± 3 forbidden transitions
27.2 days(2, 2) unstable level
(1, 0)
0 ±1 ±2 ±3 k
Ncrit ~ 200 cm-3
H3+ + H2 → (H5
+)* → H3+ + H2
Pan, Oka, ApJ 305, 518 (1986)
Oka, Shimizu2, Watson, ApJ (1971)
Oka, Epp, ApJ 613, 349 (2004)
(1, 1) ground levelCMZ and spiral arms
(3, 3) metastable level All CMZ
(2, 2) unstable level Neither
CO Mostly spiral arms
High temperature
Low density
Enter the Gemini South Observatory
The Expanding Molecular RingKaifu, Kato, Iguchi, Nature (1972)Scoville, ApJ (1972)
Whiteoak, Gardner, MNRAS (1979)
Dimension of the -100 km/s cloud
ζL = 2 ke N(H3+) (nC/nH)SV RX / f
7.3 ×10-8 cm3/s 1.6 ×10-4 1
1.6 ×1015 cm-2 3 - 10
Sodroski et al ApJ 452, 262 (1995)
ζL = (1.1 – 3.7) ×105 cm/s
ζ (s-1) L (pc)
3×10-17 (1.2 – 4.0) k3×10-16 120 – 4003×10-15 12 – 40
Oka, Geballe, Goto, Usuda, McCall, ApJ (2005)
Other stars within 30 pc
Nagata, Hyland, Straw, Sato, Kawara, ApJ 1993
Main Results so far
• Vast amount of diffuse gas• High temperature: T ~ 250 K• Low Density: n ~ 100 cm-3
• H3+ total column density: 4.3 1015 cm-2
• ¾ in CMZ, ¼ in intervening spiral arms• ½ of H3
+ in CMZ in the Expanding Mol. Ring• Pathlength ~ 100 pc• Ionization rate ~ 10-15 s-1
Volume filling factor of dense clouds 0.01
The Galactic centerThe Central Molecular Zone (CMZ)
The treasure house of H3+
Discovery of metastable H3
+
Revelation of warm and diffuse gas
Cold30 K>104 cm-3
Hot104 K~102 cm-3
Ultrahot107-8 K~0.3 cm-3
Warm250 K~102 cm-3
CO, CS X-rayH3+ Radio scattering
Volume filling factor f
0.1 0.5 - 1 ~ 0.5 «10.01
Controversies
T. Oka No hot gas in the Expanding Molecular Ring
F. Le Petit Diffuse gas cannot be that hot
J. Black Infrared pumping
(1, 0)
(3, 0)
(2, 0)
(3, 3)
F. Yusef-Zadeh 4 categories of gases ApJ 637, L101 (2006)
Linnott & Rawlings Dynamically evolving cloud A&A 448, 425 (2006)