The IRAS data base is used to locate young stellar object candidates in and near the IC 1396 complex located in the Cepheus OB2 association. Co-added survey data are used to identify all sources with a flux density Snu(100) greater than 10 Jy and with Snu(100) greater than Snu(60). The 15 sources located at the positions of globules and dark clouds are further analyzed using the in-scan slices to assess the source profiles
The Astrophysical Journal
Schwartz, Richard; Wilking, Bruce; and Giulbudagian, Armen, "A Search for Embedded Young Stellar Objects in and near the IC 1396 Complex" (1991). Physics Faculty Works. 48.
Available at: https://irl.umsl.edu/physics-faculty/48