HH24 26: structure, dynamics and chemistry

Details HH24 26: structure, dynamics and chemistry HH24 26: structure, dynamics and chemistry

Feb 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ap%26ss.224..467g&link_type=abstract

Astrophysics and Space Science, Volume 224, Issue 1-2, pp. 467-468

Astronomy and Astrophysics

Astrophysics

Molecular Clouds, Hh24&Ndash, 26, Abundances, Structure

Scientific paper

New J=1-0 HCO+ and J=2-1 C18O observations of HH24 26 reveal striking differences between these and previous maps of higher-J transitions of HCO+ and CS. The high-J HCO+ and CS emission traces the densest portions of the cloud, while C18O traces the more tenuous envelope. This is also evident in the velocity structure. HCO+ and C18O appear to be depleted from the gas phase by amounts which vary with position.

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