The detection of shocked CO emission from G 333.6-0.2.
Abstract
This paper is published as a 38 stanza poem. The main results are:In 1980, from the plane, hefound it in Orion,but no more CO could he finddespite long hours of flyin'.And so, he searched for southern sourcesof this shocked H2and found it, in G 333point six, minus, nought point two.Intensity is really weak:it's two point nought by tento the minus eighteenth power(in watts per square cm).That's thirty times as weak as wedetected in Orion.No wonder it took several yearsof concentrated tryin'.
- Publication:
-
Publications of the Astronomical Society of Australia
- Pub Date:
- 1984
- DOI:
- 10.1017/S1323358000017628
- Bibcode:
- 1984PASA....5..566S