  We present observations of near-infrared 2.12 micro-meter molecular hydrogen
outflows emerging from 1.1 mm dust continuum clumps in the North America and
Pelican Nebula (NAP) complex selected from the Bolocam Galactic Plane Survey
(BGPS). Hundreds of individual shocks powered by over 50 outflows from young
stars are identified, indicating that the dusty molecular clumps surrounding
the NGC 7000 / IC 5070 / W80 HII region are among the most active sites of
on-going star formation in the Solar vicinity. A spectacular X-shaped outflow,
MHO 3400, emerges from a young star system embedded in a dense clump more than
a parsec from the ionization front associated with the Pelican Nebula (IC
5070). Suspected to be a binary, the source drives a pair of outflows with
orientations differing by 80 degrees. Each flow exhibits S-shaped symmetry and
multiple shocks indicating a pulsed and precessing jet. The `Gulf of Mexico'
located south of the North America Nebula (NGC 7000), contains a dense cluster
of molecular hydrogen objects (MHOs), Herbig-Haro (HH) objects, and over 300
YSOs, indicating a recent burst of star formation. The largest outflow detected
thus far in the North America and Pelican Nebula complex, the 1.6 parsec long
MHO 3417 flow, emerges from a 500 Solar mass BGPS clump and may be powered by a
forming massive star. Several prominent outflows such as MHO 3427 appear to be
powered by highly embedded YSOs only visible at a wavelength > 70 micro-meters.
An `activity index' formed by dividing the number of shocks by the mass of the
cloud containing their source stars is used to estimate the relative
evolutionary states of Bolocam clumps. Outflows can be used as indicators of
the evolutionary state of clumps detected in mm and sub-mm dust continuum
surveys.
