Observational study of starless cores in Taurus

Details Observational study of starless cores in Taurus Observational study of starless cores in Taurus

Oct 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003asthe..96..546t&link_type=abstract

The Astronomical Herald (ISSN 0374-2466), Vol. 96, No. 10, p. 546 - 553 (2003)

Astronomy and Astrophysics

Astronomy

Protostars

Scientific paper

A study of star formation has been largely progressed by detections of protostars accompanying outflow phenomenon. However, there still remain a number of unresolved problems in a study of molecular condensations before protostar formation. We have carried out molecular-line observations of starless condensations in various stages in Taurus by using the 4-m telescope of Nagoya University, 45-m telescope at NRO, and 10.4m CSO telescope. In this paper, we present the important findings on the evolution of starless condensations by the statistical investigations of the observed data.

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