  We report the discovery of twelve faint Herbig-Haro (HH) objects in LDN 673
found using a novel color-composite imaging method that reveals faint H{\alpha}
emission in complex environments. Follow-up observations in [S II] confirmed
their classification as HH objects. Potential driving sources are identified
from the Spitzer c2d Legacy Program catalog and other infrared observations.
The twelve new HH objects can be divided into three groups: Four are likely
associated with a cluster of eight YSO class I/II IR sources that lie between
them; five are colinear with the T Tauri multiple star system AS 353, and are
likely driven by the same source as HH 32 and HH 332; three are bisected by a
very red source that coincides with an infrared dark cloud. We also provide
updated coordinates for the three components of HH 332. Inaccurate numbers were
given for this object in the discovery paper. The discovery of HH objects and
associated driving sources in this region provides new evidence for star
formation in the Aquila clouds, implying a much larger T Tauri population in a
seldom-studied region.
