A METHOD FOR DETERMINING THE PHYSICAL PARAMETERS OF HOT SUPERGIANTS BASED ON SPECTRAL ENERGY DISTRIBUTION ANALYSIS

A METHOD FOR DETERMINING THE PHYSICAL PARAMETERS OF HOT SUPERGIANTS BASED ON SPECTRAL ENERGY DISTRIBUTION ANALYSIS

This study determines the physical parameters of B- and A-type hot supergiants through the construction and analysis of their spectral energy distributions (SEDs). These luminous stars are in the late stages of stellar evolution and are important for understanding stellar structure and the chemical...

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Bibliographic Details
Main Authors: Alina Gyuchtash, Shakhida Nurmakhametova, Nadezhda Vaidman, Serik Khokhlov, Aldiyar Agishev, Aigerim Bakhytkyzy
Format: Article
Language:English
Published: Al-Farabi Kazakh National University 2025-06-01
Series:Physical Sciences and Technology
Online Access:https://phst.kaznu.kz/index.php/journal/article/view/523
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