Three new identifications of extended UV emission around AGB stars (2024)
- Authors:
- Autor USP: ORTIZ, ROBERTO PEREIRA - EACH
- Unidade: EACH
- DOI: 10.1093/mnras/stad3458
- Assunto: PERDA DE MASSA
- Agências de fomento:
- Language: Inglês
- Imprenta:
- Source:
- Título: Monthly Notices of the Royal Astronomical Society
- ISSN: 1365-2966
- Volume/Número/Paginação/Ano: v. v. 527, n. 3, p. 4730–4738, Jan. 2024
- Este periódico é de acesso aberto
- Este artigo NÃO é de acesso aberto
-
ABNT
GUERRERO, Martin A. e ORTIZ, Roberto Pereira. Three new identifications of extended UV emission around AGB stars. Monthly Notices of the Royal Astronomical Society, v. 527, n. Ja 2024, p. 4730–4738, 2024Tradução . . Disponível em: http://dx.doi.org/10.1093/mnras/stad3458. Acesso em: 10 fev. 2026. -
APA
Guerrero, M. A., & Ortiz, R. P. (2024). Three new identifications of extended UV emission around AGB stars. Monthly Notices of the Royal Astronomical Society, 527( Ja 2024), 4730–4738. doi:10.1093/mnras/stad3458 -
NLM
Guerrero MA, Ortiz RP. Three new identifications of extended UV emission around AGB stars [Internet]. Monthly Notices of the Royal Astronomical Society. 2024 ; 527( Ja 2024): 4730–4738.[citado 2026 fev. 10 ] Available from: http://dx.doi.org/10.1093/mnras/stad3458 -
Vancouver
Guerrero MA, Ortiz RP. Three new identifications of extended UV emission around AGB stars [Internet]. Monthly Notices of the Royal Astronomical Society. 2024 ; 527( Ja 2024): 4730–4738.[citado 2026 fev. 10 ] Available from: http://dx.doi.org/10.1093/mnras/stad3458 - Understanding high-energy (UV and X-ray) emission from AGB Stars—Episodic accretion in binary systems
- 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: 10.1093/mnras/stad3458 (Fonte: oaDOI API)
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