Distances of galactic planetary nebulae based on a relationship between the central star mass and the N/O abundance (2000)
- Authors:
- Autor USP: MACIEL, WALTER JUNQUEIRA - IAG
- Unidade: IAG
- Assunto: ASTRONOMIA
- Language: Inglês
- Imprenta:
- Source:
- Título do periódico: Revista Mexicana de Astronomía y Astrofísica
- Volume/Número/Paginação/Ano: v. 36, n. 1, p. 3-11, Abril 2000
-
ABNT
CAZETTA, J. O.; MACIEL, Walter Junqueira. Distances of galactic planetary nebulae based on a relationship between the central star mass and the N/O abundance. Revista Mexicana de Astronomía y Astrofísica, México, v. 36, n. 1, p. 3-11, 2000. -
APA
Cazetta, J. O., & Maciel, W. J. (2000). Distances of galactic planetary nebulae based on a relationship between the central star mass and the N/O abundance. Revista Mexicana de Astronomía y Astrofísica, 36( 1), 3-11. -
NLM
Cazetta JO, Maciel WJ. Distances of galactic planetary nebulae based on a relationship between the central star mass and the N/O abundance. Revista Mexicana de Astronomía y Astrofísica. 2000 ; 36( 1): 3-11. -
Vancouver
Cazetta JO, Maciel WJ. Distances of galactic planetary nebulae based on a relationship between the central star mass and the N/O abundance. Revista Mexicana de Astronomía y Astrofísica. 2000 ; 36( 1): 3-11. - Grains and the heating of hii regions
- Grains and the galactic electron temperature gradient
- Abundance gradients from disk planetary nebulae: o, 'NE', s, and 'AR'
- Nucleos de nebulosas planetarias e evolucao estelar
- Time evolution of galactic abundance gradients
- Teaching of astronomy in brasil: analyses of 1st and 2st degrees curricula
- Gravity distances of planetary nebulae
- Futuro do sol
- Determinacao de distancias de nebulosas planetarias a partir da segregacao de populacoes dos tipos de peimbert
- Radial abundance gradients in the galactic disk: observations and theory
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