Chemistry in Class 0 and I Objects

Details Chemistry in Class 0 and I Objects Chemistry in Class 0 and I Objects

Oct 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aspc..432..187c&link_type=abstract

New Horizons in Astronomy: Frank N. Bash Symposium 2009, proceedings of a conference held Oct. 18-20, 2009 in Austin, Texas, USA

Astronomy and Astrophysics

Astronomy

Scientific paper

We present a line survey of 10 Class 0 and 7 Class I protostars with 9
molecular lines. Combining dust continuum maps and molecular line maps,
we calculated the depletion factor and deuterium enhancement to study
the chemical properties. A general trend for the chemical evolution is
seen: higher deuterium fractionation at higher CO depletion.

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