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Bipolar molecular outflows

Andr4 P., Ward-Thompson, D., and Baisony, M. (2000). Prom Pre-Stellar Cores to Protostars The Initial Conditions of Star Eormation. In Protostars and Planets IV (V. Mannings, A. P. Boss, and S. S. Russell, eds.), in press. University of Arizona Press, Tucson, AZ. Bachiller, R. (1996). Bipolar molecular outflows from young stars and protostars, Ann. Rev. Astron. Astrophys. 34,111-154. [Pg.195]

DO PRE-MAIN-SEQUENCE STARS DRIVE BIPOLAR MOLECULAR OUTFLOWS ... [Pg.121]

Spectacular H2 images of the highly collimated, clumpy, bipolar L1448 molecular jet (Bally, Lada, and Lane 1993) show a complex structure. The H2 emission generally outlines the structure of the cooling gas behind radiative shocks produced by the interaction of energetic YSO jets/outflows with the ambient molecular gas. In this case, the knots are interpreted in terms of shocks associated with nun-wave buUets . [Pg.6]

See other pages where Bipolar molecular outflows is mentioned: [Pg.153]    [Pg.42]    [Pg.171]    [Pg.98]    [Pg.153]    [Pg.42]    [Pg.171]    [Pg.98]    [Pg.68]    [Pg.43]    [Pg.169]    [Pg.121]    [Pg.240]    [Pg.668]    [Pg.502]    [Pg.311]   
See also in sourсe #XX -- [ Pg.42 ]



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