Astronomy and Astrophysics – Astronomy
Scientific paper
Sep 1998
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998apj...504..866s&link_type=abstract
Astrophysical Journal v.504, p.866
Astronomy and Astrophysics
Astronomy
10
Ism: Globules, Ism: Molecules, Molecular Processes, Radio Lines: Ism, Stars: Pre-Main-Sequence
Scientific paper
A sample of 14 small Bok globules and of eight Herbig Ae/Be stars has been observed in the molecular rotational lines of HCO+, HCN, HNC, N2H+, and C2H at 3 mm wavelength. The observational results have been used together with a pseudo-time-dependent chemical model to study the evolution of a molecular cloud toward the formation of a low-mass star. The new chemical and physical scenario that is inferred from the molecular line data is discussed in relation with the existing literature data obtained from infrared to far-infrared data.
Casolari A.
Cecchi-Pestellini Cesare
Fanti Carla
Olberg Michael
Scappini Flavio
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