| Name: Raksha S Affiliation: CHRIST (Deemed to be University) Conference ID: ASI2023_382 Title : Why do we see hot-emission stars at high galatic latitude? Authors and Co-Authors : Raksha S, Blesson Mathew, Sreeja S. Kartha, Shridharan B, Ujjwal K Abstract Type : Poster Abstract Category : Stars, ISM and Galaxy Abstract : Stars are usually found in associations in the active star-forming region. It is rare to find stars away from any molecular clouds, and in the regions high above the Galactic plane. High-latitude clouds (|b| >30°) are predominantly diffused or translucent. Thus, these low-density environments at high latitudes create a challenge for the formation of hot stars, as they are not convenient sites for star formation. We choose a sample of 40 high galactic latitude emission-line stars (Shridharan et al. 2021) of spectral type B and A. By analyzing the dynamics of these stars, a comprehensive understanding on the formation is made. Through the trace back analysis we evaluated the formation region of these stars. |