| 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 : | Raksha S, Blesson Mathew, Sreeja S. Kartha, Shridharan B, Ujjwal K |
| Mode of Presentation: | 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. |
