Modelling the disc around the primary star of the X-ray binary system: MT91-213 (2024)
- Authors:
- Autor USP: CARCIOFI, ALEX CAVALIERI - IAG
- Unidade: IAG
- DOI: 10.1093/mnras/stae1950
- Assunto: ESTRELAS BINÁRIAS
- Agências de fomento:
- Language: Inglês
- Imprenta:
- Source:
- Título: Monthly Notices of the Royal Astronomical Society
- ISSN: 0035-8711
- Volume/Número/Paginação/Ano: v.533, p.2867-2875, 2024
- Este periódico é de acesso aberto
- Este artigo NÃO é de acesso aberto
-
ABNT
GHOREYSHI, M. R e JONES, C. E. e CARCIOFI, Alex Cavaliéri. Modelling the disc around the primary star of the X-ray binary system: MT91-213. Monthly Notices of the Royal Astronomical Society, v. 533, p. 2867-2875, 2024Tradução . . Disponível em: https://doi.org/10.1093/mnras/stae1950. Acesso em: 22 jan. 2026. -
APA
Ghoreyshi, M. R., Jones, C. E., & Carciofi, A. C. (2024). Modelling the disc around the primary star of the X-ray binary system: MT91-213. Monthly Notices of the Royal Astronomical Society, 533, 2867-2875. doi:10.1093/mnras/stae1950 -
NLM
Ghoreyshi MR, Jones CE, Carciofi AC. Modelling the disc around the primary star of the X-ray binary system: MT91-213 [Internet]. Monthly Notices of the Royal Astronomical Society. 2024 ;533 2867-2875.[citado 2026 jan. 22 ] Available from: https://doi.org/10.1093/mnras/stae1950 -
Vancouver
Ghoreyshi MR, Jones CE, Carciofi AC. Modelling the disc around the primary star of the X-ray binary system: MT91-213 [Internet]. Monthly Notices of the Royal Astronomical Society. 2024 ;533 2867-2875.[citado 2026 jan. 22 ] Available from: https://doi.org/10.1093/mnras/stae1950 - Short-term variablility and mass loss in Be stars: II. Physical taxonomy of photometric variability observed by the Kepler spacecraft
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Informações sobre o DOI: 10.1093/mnras/stae1950 (Fonte: oaDOI API)
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