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H 2 S 2. March 28-31, 1966, APS Durham, NC. April 22, 1966, Invitation to give a seminar. October, 1970. Scrutiny of the Central Parsec of the Galactic Center by Infrared Spectra of H 3 + and 13 CO: GCIRS 3 and GCIRS 1W. Miwa Goto, Max-Planck-Institute for Astronomy, Heidelberg

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October 1970

H2S2

March 28-31, 1966, APS Durham, NC

April 22, 1966, Invitation to give a seminar

October, 1970


October 1970

Scrutiny of the Central Parsec of the Galactic Center by Infrared Spectra of H3+ and 13CO: GCIRS 3 and GCIRS 1W

Miwa Goto, Max-Planck-Institute for Astronomy, Heidelberg

Tomonori Usuda, Subaru Telescope, Hilo

Thomas R. Geballe, Gemini Observatory, Hilo

Farhad Yusef-Zadeh, Northwestern University, Evanston

Nick Indriolo, and Ben J. McCall,

University of Illinois at Urbana-Champaign, Urbana

Takeshi Oka, University of Chicago, Chicago

Harvey Liszt, National Radio Astronomy Observatory

66th OSU International Symposium, June 21, 2011


October 1970

T Infrared Spectra of H ~ 250 K

n < 100 cm-3

L > 2.2  105 cm/s

 = 2  10-15 s-1 L > 35pc

GCS 3-2

Oka, Geballe, Goto, Usuda, McCall, 2005, ApJ, 632, 882

,  Geballe, Oka, 2010, ApJ, 709, L70

ε+

ε-

η+

λ

α+

θ+

θ-

δ+

Goto, Usuda, Nagata, Geballe, McCall, Indriolo,

Suto, Henning, Morong, Oka, 2008, ApJ, 688, 306

30 pc


October 1970

Molecular face-on view of the GC Infrared Spectra of H

R ~ 180 pc

101 pc

130 pc

Reid, Menten, Zheng, Brunthaler, Xu, ApJ, 2009

The Expanding Molecular Ring

T. Sawada et al. 2001

T. Sawada et al. 2004

N. Z. Scoville, 1972



October 1970

The Central Cluster Infrared Spectra of H

8.4” 0.33 pc

The ISAAC L-band image of the Galactic center showing most of the named sources (from Viehmann et al. 2005)


October 1970

H Infrared Spectra of H3+ and 13CO spectra toward GCIRS 3 and GCIRS 1W

Warm and diffuse gas

(3,3)

(2,2)

361 K

27 days

(1,1)


October 1970

H Infrared Spectra of H3+ and 13CO spectra toward GCIRS 3 and GCIRS 1W

Velocity profiles and radial location of gas

 140 km s-1

Subtract spiral arms

Expanding Mol. Ring

Inner Molecular gas


October 1970

Dense cloud near Sgr A* toward GCIRS 3 Infrared Spectra of H

N(1,1) = 1.89 ± 0.31 cm-2

N(2,2) = 2.05 ± 0.57 cm-2

N(3,3) = 2.78 ± 0.30 cm-2

T ~ 300 K


October 1970

Ionization Infrared Spectra of H rate

L = 2 keN(H3+) (nC/nH)SV RX / f(H2)

1.8 ×10-9 cm3/s

1.6 ×10-4

1

L = 2 kLN(H3+) (nC/nH)SV RX / f(H2)

1.0 ×1015 cm-2

3

~ 1700 cm s-1

if L = 0.5 pc, = 1.1  10-15 s-1


October 1970

Ubiquity of Infrared Spectra of HH3+

Sgr A* to 30 pc East

Goto, et al. 2008, ApJ, 688, 306

30 pc