Origin of mg II absorption-line systems of quasi-stellar objects (1993)
- Authors:
- USP affiliated authors: VIEGAS, SUELI MARIA MARINO - IAG ; GRUENWALD, RUTH BOMFIM - IAG
- Unidade: IAG
- Assunto: ASTRONOMIA
- Language: Inglês
- Imprenta:
- Source:
- Título do periódico: Astrophysical Journal
- Volume/Número/Paginação/Ano: v. 415, n. 2 pt. 1, p. 534-540, out. 1993
-
ABNT
GRUENWALD, Ruth Bomfim e VIEGAS, Sueli Maria Marino. Origin of mg II absorption-line systems of quasi-stellar objects. Astrophysical Journal, v. 415, n. 2 pt. 1, p. 534-540, 1993Tradução . . Acesso em: 29 mar. 2024. -
APA
Gruenwald, R. B., & Viegas, S. M. M. (1993). Origin of mg II absorption-line systems of quasi-stellar objects. Astrophysical Journal, 415( 2 pt. 1), 534-540. -
NLM
Gruenwald RB, Viegas SMM. Origin of mg II absorption-line systems of quasi-stellar objects. Astrophysical Journal. 1993 ; 415( 2 pt. 1): 534-540.[citado 2024 mar. 29 ] -
Vancouver
Gruenwald RB, Viegas SMM. Origin of mg II absorption-line systems of quasi-stellar objects. Astrophysical Journal. 1993 ; 415( 2 pt. 1): 534-540.[citado 2024 mar. 29 ] - Effect of relativistic electrons on the narrow emission lines of agn
- Balmer lines in active galactic nuclei
- Influence of relativistic electrons on a photoionized gaseous cloud
- On warmes as the ionizing source in agn
- Theoretical and empirical abundance determination in gaseous nebulae
- Origin of the quasi-stellar object absorption lines
- Nebulosas planetárias: super-abundância de N ou efeitos de geometria?
- Ionization corrections for low-metallicity 'H' II regions and the primordial helium abundance
- Morphology and kinematics of planetary nebulae. II. a diabolo model for NGC 3132
- Temperature fluctuations in pn
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