'30 pc' presentation slideshows

Star formation under extreme conditions: the Galactic center

Revelation of a vast amount of warm (~ 250 K) and diffuse (? 100 cm -3 ) gas and high ionization rate ( ? > 10 -15 s -1 ) in the Central Molecular Zone by the Infrared Spectrum of H 3 + Takeshi Oka Department of Astronomy and Astrophysics and Department of Chemistry

279 views • 21 slides

H 3 + in the Central Molecular Zone of the Galactic Center: Revelation of a New Category of Gas

H 3 + in the Central Molecular Zone of the Galactic Center: Revelation of a New Category of Gas. Takeshi Oka. Department of Astronomy and Astrophysics and Department of Chemistry, The Enrico Fermi Institute, University of Chicago. Tom Geballe Gemini Observatory.

276 views • 20 slides

H 3 +

H 3 +. H 3 + , a new astrophysical probe: Revelation of warm and diffuse gas near the Galactic center. Takeshi Oka Department of Astronomy and Astrophysics and Department of Chemistry, The Enrico Fermi Institute The University of Chicago. Thomas R. Geballe Gemini Observatory

336 views • 18 slides

Revelation of a vast amount of warm and diffuse gas and high ionization rate

Revelation of a vast amount of warm and diffuse gas and high ionization rate in the Central Molecular Zone of the Galactic center by the Infrared Spectrum of H 3 + Takeshi Oka Department of Astronomy and Astrophysics and Department of Chemistry

265 views • 17 slides

H 3 +

H 3 +. Search for hot and bright stars for H 3 + spectroscopy Near the Galactic center. Takeshi Oka. Department of Astronomy and Astrophysics and Department of Chemistry The Enrico Fermi Institute, University of Chicago. and T. R. Geballe. Gemini Observatory.

262 views • 16 slides

Warm and Diffuse Gas and High Ionizzation Rate Near the Galactic Center

Warm and Diffuse Gas and High Ionizzation Rate Near the Galactic Center from 140 pc West to 85 pc East of Sgr A*. Takeshi Oka , Chris MORONG, University of Chicago, Chicago Tom Geballe, Gemini Observatory, Hilo Nick Indriolo, Ben McCall, University of Illinois at Urbana-Champaign, Urbana

255 views • 14 slides

October, 1970

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

241 views • 14 slides

Spectroscopy of H 3 + and CO toward the Galactic center

Spectroscopy of H 3 + and CO toward the Galactic center. Takeshi Oka , Christopher P. Morong, Department of Astronomy And Astrophysics and Department of Chemistry University of Chicago Thomas R. Geballe, Gemini Observatory, Hilo, Hawaii

208 views • 13 slides

Debris Disk Studies with CCAT

310 views • 12 slides

Bally et al. 2010, ApJ, 721, 137

240 views • 12 slides

Forward Contracts - RBI Guidelines

Forward Contracts - RBI Guidelines. What is a Forward Contract? It is an agreement to buy or sell a specified quantity of an asset at a certain future date for a certain price agreed upon now. Contracted Exposures -

294 views • 7 slides