Cj. Lada et M. Fich, THE STRUCTURE AND ENERGETICS OF A HIGHLY COLLIMATED BIPOLAR OUTFLOW -NGC 2264G, The Astrophysical journal, 459(2), 1996, pp. 638-652
We present a detailed observational study of (CO)-C-12 (J = 2-->1) emi
ssion from the spectacular bipolar molecular outflow NGC 2264G. These
observations enable us to make significantly improved determinations o
f the basic physical parameters of the outflow and reveal rich structu
ral detail in both its spatial morphology and velocity field. We ident
ify a number of robust physical characteristics of the outflow that pr
ovide critical challenges for the development of a theoretical underst
anding of the dynamical nature of this and other bipolar molecular out
flows. In particular, we find that (1) the velocity field of the outfl
ow is described by a single ''Hubble'' law to a remarkable degree of p
recision over its entire extent, (2) the flow exhibits a high degree o
f bipolarity with an intensity contrast between red and blue emission
in each lobe of at least a factor of 20, which indicates that the moti
on of gas in the outflow is strongly (forwardly) directed along the fl
ow major axis, (3) the flow exhibits a well-behaved power-law variatio
n of mass with velocity, and (4) the collimation of the flow increases
systematically with flow velocity and distance from the driving sourc
e, with the highest velocity gas very jetlike in appearance. Moreover,
at the highest flow velocities the two oppositely directed lobes disp
lay a high degree of similarity in their basic physical properties sug
gesting that the underlying wind driving the outflow is characterized
by an intrinsic bipolar symmetry which originates with the driving eng
ine at the origin of the outflow. Existing outflow theory cannot yet a
ccount for the constraints imposed by these observations. In particula
r, we find the general result that bow shock models cannot produce the
degree of bipolarity required to match the observations of this and o
ther outflows. Improved estimates of the outflow's mass, size, and ene
rgetics provide strong constraints on the energetics of the driving en
gine.