Grain formation in post-shocked wind collisions of massive binary systems (2003)
Source: A massive star odyssey: from main sequence to supernova. Conference titles: Symposium of the International Astronomical Union. Unidade: IAG
Assunto: MEIO INTERESTELAR
ABNT
FALCETA-GONÇALVES, Diego e JATENCO-PEREIRA, Vera e ABRAHAM, Zulema. Grain formation in post-shocked wind collisions of massive binary systems. 2003, Anais.. San Francisco: ASP, 2003. . Acesso em: 18 nov. 2024.APA
Falceta-Gonçalves, D., Jatenco-Pereira, V., & Abraham, Z. (2003). Grain formation in post-shocked wind collisions of massive binary systems. In A massive star odyssey: from main sequence to supernova. San Francisco: ASP.NLM
Falceta-Gonçalves D, Jatenco-Pereira V, Abraham Z. Grain formation in post-shocked wind collisions of massive binary systems. A massive star odyssey: from main sequence to supernova. 2003 ;[citado 2024 nov. 18 ]Vancouver
Falceta-Gonçalves D, Jatenco-Pereira V, Abraham Z. Grain formation in post-shocked wind collisions of massive binary systems. A massive star odyssey: from main sequence to supernova. 2003 ;[citado 2024 nov. 18 ]