- Startpagina tijdschrift
- Volume 93 - Année 2024
- No 2 - Proceeedings of the 3rd BINA Workshop on th...
- Evolution and Final Fates of a Rotating 25M⊙ Pop III Star
    
                      
                
                sinds 05 februari 2011 :
                                  Weergave(s): 285                                      (8 ULiège)
                                      Download(s): 11                                      (0 ULiège)
               
         
          
         
                           Amar 
Aryan, Shashi Bhushan 
Pandey, Rahul 
Gupta, Sugriva Nath 
Tiwari & Amit Kumar 
Ror                                Evolution and Final Fates of a Rotating 25M⊙ Pop III Star                    
                        (Volume 93 - Année 2024 — No 2 - Proceeedings of the 3rd BINA Workshop on the Scientific Potential of the Indo-Belgian Cooperation)
                    
                          
                                                          Article                                    
        
          
                                     
          Abstract
        
          In this manuscript, we present the one-dimensional stellar evolution of two rotating population III (Pop III) star models, each having a mass of 25M⊙ at the zero-age main-sequence (ZAMS). The slowly rotating model has an initial angular rotational velocity of 10% of the critical angular rotational velocity. In contrast, the rapidly rotating model has an initial angular rotational velocity of 70% of the critical angular rotational velocity. As an effect of rotationally enhanced mixing, we find that the rapidly rotating model suffers an enormous mass loss due to the deposition of a significant amount of CNO elements toward the surface after the main-sequence phase. We also display the simulated light curves as these models explode into core-collapse supernovae (CCSNe).
                     
            Keywords : Population III stars, Stellar evolution, Hydrodynamic simulation, Supernovae
                                                   
                                                                                                                                
          Om dit artikel te citeren:
            
                          Amar Aryan, Shashi Bhushan Pandey, Rahul Gupta, Sugriva Nath Tiwari & Amit Kumar Ror, «Evolution and Final Fates of a Rotating 25M⊙ Pop III Star», Bulletin de la Société Royale des Sciences de Liège [En ligne],                Volume 93 - Année 2024,                No 2 - Proceeedings of the 3rd BINA Workshop on the Scientific Potential of the Indo-Belgian Cooperation,      700-708  URL : http://popups.ulg.be/0037-9565/index.php?id=11843.             
             
           
          Aryabhatta Research Institute of observational sciencES (ARIES), Nainital, Uttarakhand, India-263001 and Department of Physics, Deen Dayal Upadhyaya Gorakhpur University, Gorakhpur, Uttar Pradesh, India-273009. Corresponding author: amararyan941@gmail.com and amar@aries.res.in
 
           
          Aryabhatta Research Institute of observational sciencES (ARIES), Nainital, Uttarakhand, India-263001
 
           
          Aryabhatta Research Institute of observational sciencES (ARIES), Nainital, Uttarakhand, India-263001 and Department of Physics, Deen Dayal Upadhyaya Gorakhpur University, Gorakhpur, Uttar Pradesh, India-273009
 
           
          Department of Physics, Deen Dayal Upadhyaya Gorakhpur University, Gorakhpur, Uttar Pradesh, India-273009
 
           
          Aryabhatta Research Institute of observational sciencES (ARIES), Nainital, Uttarakhand, India-263001