Integral field unit spectroscopy of 10 early-type galactic nuclei: I. Principal component analysis Tomography and nuclear activity (2014)
- Authors:
- Autor USP: STEINER, JOAO EVANGELISTA - IAG
- Unidade: IAG
- DOI: 10.1093/mnras/stu441
- Subjects: ESPECTROSCOPIA; GALÁXIAS ATIVAS; GALÁXIAS ELÍPTICAS; ESTATÍSTICA; GALÁXIAS
- Language: Inglês
- Imprenta:
- Source:
- Título: Monthly Notices of the Royal Astronomical Society
- ISSN: 0035-8711
- Volume/Número/Paginação/Ano: v. 440, p. 2419-2441, 2014
- Status:
- Artigo possui acesso gratuito no site do editor (Bronze Open Access)
- Versão do Documento:
- Versão publicada (Published version)
- Acessar versão aberta:
-
ABNT
RICCI, T. V e STEINER, João Evangelista e MENEZES, R.B. Integral field unit spectroscopy of 10 early-type galactic nuclei: I. Principal component analysis Tomography and nuclear activity. Monthly Notices of the Royal Astronomical Society, v. 440, p. 2419-2441, 2014Tradução . . Disponível em: https://doi.org/10.1093/mnras/stu441. Acesso em: 18 mar. 2026. -
APA
Ricci, T. V., Steiner, J. E., & Menezes, R. B. (2014). Integral field unit spectroscopy of 10 early-type galactic nuclei: I. Principal component analysis Tomography and nuclear activity. Monthly Notices of the Royal Astronomical Society, 440, 2419-2441. doi:10.1093/mnras/stu441 -
NLM
Ricci TV, Steiner JE, Menezes RB. Integral field unit spectroscopy of 10 early-type galactic nuclei: I. Principal component analysis Tomography and nuclear activity [Internet]. Monthly Notices of the Royal Astronomical Society. 2014 ; 440 2419-2441.[citado 2026 mar. 18 ] Available from: https://doi.org/10.1093/mnras/stu441 -
Vancouver
Ricci TV, Steiner JE, Menezes RB. Integral field unit spectroscopy of 10 early-type galactic nuclei: I. Principal component analysis Tomography and nuclear activity [Internet]. Monthly Notices of the Royal Astronomical Society. 2014 ; 440 2419-2441.[citado 2026 mar. 18 ] Available from: https://doi.org/10.1093/mnras/stu441 - NGC 6744: a nearby Milky Way twin with a very low-luminosity AGN
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