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Low velocity shock-cloud encounters II.
Authors:L Viktor Tóth  András Horváth Jr  Lauri K Haikala
Institution:(1) Loránd Eötvös University, Budapest, Hungary;(2) Helsinki University Observatory, Finland;(3) Present address: Széchenyi István College, Gyodblacr, Hungary
Abstract:We report on a comparative study of nearby shocked clouds with and without star formation, based on IRAS, HI(21cm), CO(1-0) NH3 (and other molecular line) observations. The dark clouds L1780 (no star formation) and L1251 (high SFE) are discussed here. Their density and velocity structure are compared with the predictions of the HD model of Horváth & Tóth (1995), Paper I.
Keywords:Molecular Clouds  Interstellar Shocks
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