B and V photometry of the metal-rich bulge globular cluster NGC 6304 (2000)
- Authors:
- USP affiliated author: BARBUY, BEATRIZ LEONOR SILVEIRA - IAG
- School: IAG
- Subjects: ASTRONOMIA; ASTROFÍSICA ESTELAR
- Language: Inglês
- Imprenta:
- Source:
- Título do periódico: Astronomy and Astrophysics
- ISSN: 0004-6361
- Volume/Número/Paginação/Ano: v. 357, n. 2, p. 495-500, May 2000
-
ABNT
ORTOLANI, S et al. B and V photometry of the metal-rich bulge globular cluster NGC 6304. Astronomy and Astrophysics, v. 357, n. 2, p. 495-500, 2000Tradução . . Acesso em: 03 jul. 2022. -
APA
Ortolani, S., Momany, Y., Bica, E., & Barbuy, B. L. S. (2000). B and V photometry of the metal-rich bulge globular cluster NGC 6304. Astronomy and Astrophysics, 357( 2), 495-500. -
NLM
Ortolani S, Momany Y, Bica E, Barbuy BLS. B and V photometry of the metal-rich bulge globular cluster NGC 6304. Astronomy and Astrophysics. 2000 ; 357( 2): 495-500.[citado 2022 jul. 03 ] -
Vancouver
Ortolani S, Momany Y, Bica E, Barbuy BLS. B and V photometry of the metal-rich bulge globular cluster NGC 6304. Astronomy and Astrophysics. 2000 ; 357( 2): 495-500.[citado 2022 jul. 03 ] - VLT-UVES Spectroscopy of the subgiant I-24 of the bulge globular cluster NGC 6528 in baade´s window
- Mapping out the interstellar extinction in the central 10 degrees of the galaxy with 2MASS
- New infrared star clusters in the Northern and Equatorial milky way with 2MASS
- First stars V - Abundance patterns from C to Zn and supernova yields in the early galaxy*,*
- Lead abundance in the uranium star CS 31082-001
- Aglomerados globulares das nuvens de Magalhães: idade e metalicidades
- A new approach to derive ['alfa'/Fe] for integrated stellar populations
- Metal-poor globular clusters of the galactic bulge
- Physical parameters of intermediate-age LMC clusters from modelling of HST CMDs
- The distance and space distribution of bulge globular clusters
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