Sahai, Raghvendra 
; Sanz Forcada, Jorge ; Guerrero, Martín A ; Ortiz, Roberto Pereira ; Sanchez Contreras, Carmen
Source: Galaxies. Unidade: EACH
Subjects: ASTROFÍSICA ESTELAR, ESTRELAS BINÁRIAS, EVOLUÇÃO ESTELAR, RAIOS CÓSMICOS, PERDA DE MASSA, RAIOS X
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SAHAI, Raghvendra et al. Understanding high-energy (UV and X-ray) emission from AGB Stars—Episodic accretion in binary systems. Galaxies, v. 10, n. 3, p. art. 62 [ 01-10], 2022Tradução . . Disponível em: https://doi.org/10.3390/galaxies10030062. Acesso em: 05 jun. 2024.APA
Sahai, R., Sanz Forcada, J., Guerrero, M. A., Ortiz, R. P., & Sanchez Contreras, C. (2022). Understanding high-energy (UV and X-ray) emission from AGB Stars—Episodic accretion in binary systems. Galaxies, 10( 3), art. 62 [ 01-10]. doi:10.3390/galaxies10030062NLM
Sahai R, Sanz Forcada J, Guerrero MA, Ortiz RP, Sanchez Contreras C. Understanding high-energy (UV and X-ray) emission from AGB Stars—Episodic accretion in binary systems [Internet]. Galaxies. 2022 ; 10( 3): art. 62 [ 01-10].[citado 2024 jun. 05 ] Available from: https://doi.org/10.3390/galaxies10030062Vancouver
Sahai R, Sanz Forcada J, Guerrero MA, Ortiz RP, Sanchez Contreras C. Understanding high-energy (UV and X-ray) emission from AGB Stars—Episodic accretion in binary systems [Internet]. Galaxies. 2022 ; 10( 3): art. 62 [ 01-10].[citado 2024 jun. 05 ] Available from: https://doi.org/10.3390/galaxies10030062
