Observations of High CO Rotational Lines in Post-AGBs and PN

Details Observations of High CO Rotational Lines in Post-AGBs and PN Observations of High CO Rotational Lines in Post-AGBs and PN

Feb 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ap%26ss.224..305j&link_type=abstract

Astrophysics and Space Science, Volume 224, Issue 1-2, pp. 305-308

Astronomy and Astrophysics

Astrophysics

Molecular Processes, Shock Waves, Stars : Agb And Post-Agb

Scientific paper

We present a preliminary interpretation of high CO rotational line data
obtained from KAO. The possibility of either a PDR or a shock model is
considered in order to explain the observations.

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