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We present {\it Spitzer} images of the relatively sparse, low luminosityyoung cluster L988e, as well as complementary near-infrared (NIR) andsubmillimeter images of the region. The cluster is asymmetric, with the westernregion of the cluster embedded within the molecular cloud, and the slightlyless dense eastern region to the east of, and on the edge of, the molecularcloud. With these data, as well as with extant H$\alpha$ data of starsprimarily found in the eastern region of the cluster, and a molecular $^{13}$COgas emission map of the entire region, we investigate the distribution offorming young stars with respect to the cloud material, concentratingparticularly on the differences and similarities between the exposed andembedded regions of the cluster. We also compare star formation in this regionto that in denser, more luminous and more massive clusters already investigatedin our comprehensive multi-wavelength study of young clusters within 1 kpc ofthe Sun.

Spitzer, Near-Infrared, and Submillimeter Imaging of the Relatively Sparse Young Cluster, Lynds 988e