Understanding high-energy (UV and X-ray) emission from AGB Stars—Episodic accretion in binary systems (2022)
- Authors:
- Autor USP: ORTIZ, ROBERTO PEREIRA - EACH
- Unidade: EACH
- DOI: 10.3390/galaxies10030062
- Subjects: ASTROFÍSICA ESTELAR; ESTRELAS BINÁRIAS; EVOLUÇÃO ESTELAR; RAIOS CÓSMICOS; PERDA DE MASSA; RAIOS X
- Language: Inglês
- Imprenta:
- Source:
- Este periódico é de acesso aberto
- Este artigo NÃO é de acesso aberto
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ABNT
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: 11 fev. 2026. -
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/galaxies10030062 -
NLM
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 2026 fev. 11 ] Available from: https://doi.org/10.3390/galaxies10030062 -
Vancouver
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 2026 fev. 11 ] Available from: https://doi.org/10.3390/galaxies10030062 - Three new identifications of extended UV emission around AGB stars
- Ultraviolet emission from main-sequence companions of AGB stars
- Y Gem, a symbiotic star outshone by its asymptotic giant branch primary component
- Detailed studies of IPHAS sources – II. Sab 19, a true planetary nebula and its mimic crossing the Perseus Arm
- The effect of pulsation on the near-ultraviolet spectrum of AGB stars
- X-Ray AGB Stars in the 4XMM-DR9 Catalog: Further Evidence for Companions
- CGCS 6306, another X-ray-emitting asymptotic giant branch star confirmed to be a symbiotic binary
- A large bubble around the AGB star R Dor detected in the UV
- Space Velocity and Time Span of Jets in Planetary Nebulae
- Asymptotic giant branch stars in the eROSITA-DE eRASS1 catalog
Informações sobre o DOI: 10.3390/galaxies10030062 (Fonte: oaDOI API)
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