Observation of H3+ in Dense and Diffuse Clouds

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Table of Contents

Why Study H3+?

Formation of H3+

H3+ Destruction

H3+ Number Density

H3+ in Dense Clouds

Dense Cloud Detections

Cloud Parameter Estimates

Dense Cloud Results

H3+ in Diffuse Clouds!

Infrared CO

Diffuse Cloud Parameters

Galactic Center

 Authors: Ben McCall, Tom Geballe, Ken Hinkle, Takeshi Oka 

Email: bjmccall@astro.berkeley.edu

Home Page: http://astro.berkeley.edu/~bjmccall

Other information:
Presented at the 193rd Meeting of the American Astronomical Society in Austin, TX, 1999. 

Download presentation source 

View abstract in the Bulletin of the AAS