This work presents a multiwavelength study of the Auriga region. It includes the investigation of the evolutionary stages, disk properties and other parameters like Temperature, Mass etc. of Young Stellar Objects (YSOs) across the Auriga region by modeling the broadband optical to mid-infrared (MIR) Spectral Energy Distributions (SEDs). The YSOs are classified
into different classes based on the parameters determined from their SED response (Robitaille
et al.,2007) and are then being compared with the Classes obtained from near infrared (NIR)
to mid infrared (MIR) spectral indices α to test the robustness of the SED model. Mass and
age of the YSOs calculated from the modeling has been compared with the values obtained
from optical Color Magnitude Diagram analysis. The spatial distribution of Class I & FLAT
class predicts triggered star formation.