Multiwavelength Study of High-mass Star Forming Region G320.2325−0.2844 Using MeerKAT, ALMA, Spitzer and Gaia

Project Description:

Observational study of high-mass star forming regions is gaining more interest and attention because of improved sensitivity and angular resolution offered by newly developed and upgraded instruments around the world. Understanding the formation processes of high-mass stars is very challenging from observational point of view due to the elusive nature of massive protostars. This project will investigate the multiwavelength nature of G320.2325−0.2844 star forming region using MeerKAT, ALMA, Spitzer and Gaia Data, with the aim of characterizing the physical, chemical and kinematic properties of the region. The study will provide valuable insight into the observed evolutionary stages of high-mass star forming regions which has been a subject of astronomical interest. The radio properties of the region will be obtained from the MeerKAT data. The ALMA data will provide the chemical and kinematic properties of the region. The infrared and optical properties of the region will be provided from the Spitzer and Gaia data. Combining the results of these observations will enable one to reconstruct the evolutionary stages of high-mass star forming region.

Research Area:

Astronomy

Project Level:

Masters

This Project Is Offered At The Following Node(s):

(UCT)(UKZN)(NWU)

Special Requirements:

Good python programming skills and experience in the use of CASA software will be an added advantage. However, student without prior skills and experience will acquire the skills during the study.