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To: AntiJen
I try NOW to listen to them, especially after the last experience..........all's I can say now is:
"Better living, thru chemistry".
292 posted on 08/22/2002 6:34:20 PM PDT by tomkow6
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To: tomkow6; RadioAstronomer; Sabertooth
"Better living, thru chemistry".

Oh, did you learn that yesterday from RA and Sabertooth?

**********
From RA's science post: Radio astronomers use CO emissions at 1.3 and 2.6 mm to identify molecular hydrogen (H2) in these cold molecular clouds. H I regions consist primarily of neutral atomic hydrogen (H) gas with densities of up to 107 atoms per cubic meter at temperatures around 100 K, and are detected from 21-cm emissions generated by the quantum spin flip of individual hydrogen electrons.

Sabertooth to RA: True enough, but things really get interesting as the radio astronomers delve into the mass adenoidal transfusions of C17H21NO4.

320 posted on 08/22/2002 6:51:07 PM PDT by Jen
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