Interferometric studies of low-mass protostars

Details Interferometric studies of low-mass protostars Interferometric studies of low-mass protostars

May 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011iaus..280e...3j&link_type=abstract

The Molecular Universe, Proceedings of the 280th Symposium of the International Astronomical Union held in Toledo, Spain, May 30

Astronomy and Astrophysics

Astronomy

Scientific paper

Deeply embedded protostars provide an important laboratory for studying the chemistry of star formation - providing the link between dense regions in molecular clouds from which stars are formed, i.e., the initial conditions and the end product in terms of, e.g., disk and planet formation. High angular resolution observations at (sub)millimeter wavelengths provide an important tool for studying the chemical composition of such low-mass protostars. They for example contrain the spatial molecular abundance variations - and can thereby identify which species are useful tracers of different components of the protostars at different evolutionary stages. In this talk I will discuss the results on the chemical evolution of low-mass protostars from high angular resolution (sub)millimeter interferometric observations.

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