Beatriz Barbuy
机构: Universidade de São Paulo - IAG, Rua do Matao 1226, 05508-090 Sao Paulo, Brazil
每年引用次数
引用次数
引用: 27,832
H-指数: 81
I10-指数 : 305
出版物: 1,041
Type I planetary nebulae in the Large Magellanic Cloud: oxygen, sulphur and argon abundances as tracers of chemical enrichment.
T. E. P. Idiart , J. A. De Freitas Pacheco , R. D. D. Costa , B. Barbury
Astronomy and Astrophysics 271 ( 2) 429 -434
2
1993
Carbon and nitrogen abundances in metal-poor dwarfs of the solar neighborhood.
Duane F. Carbon , Beatrice Barbuy , Robert P. Kraft , Eileen D. Friel
Publications of the Astronomical Society of the Pacific 99 ( 615) 335 -368
115
1987
The metal-rich bulge globular cluster NGC 6401
Eduardo Luiz Damiani Bica , S. Desidera , Beatriz Barbuy , Sergio Ortolani
Astronomy and Astrophysics 348 ( 3) 783 -788
1
1999
NTT VI photometry of the metal-rich and obscured bulge globular cluster Terzan 5*
Eduardo Luiz Damiani Bica , Beatriz Barbuy , Sergio Ortolani
Astronomy and Astrophysics 308 ( 3) 733 -737
3
1996
Metallicity of the star III-17 in the bulge globular cluster NGC 6553.
Eduardo Luiz Damiani Bica , Beatriz Barbuy , Sergio Ortolani , S. Castro
Astronomy and Astrophysics 259 ( 2) 607 -613
1992
HST observations of Terzan 1: a second parameter globular cluster in the galactic bulge
Eduardo Luiz Damiani Bica , Roberto Gilmozzi , Alvio Renzini , Beatriz Barbuy
Astronomy and Astrophysics 350 ( 3) 840 -846
2
1999
Metal-rich globular clusters : giant branch morphology as a metallicity Criterion
Eduardo Luiz Damiani Bica , Beatriz Barbuy , Sergio Ortolani
Astronomy and Astrophysics 249 ( 2)
1991
NTT V, I and Gunn Z colour-magnitude diagrams of Liller 1: a globular cluster as metal-rich as the inner bulge stellar population?
Eduardo Luiz Damiani Bica , Beatriz Barbuy , Sergio Ortolani
Astronomy and Astrophysics 306 ( 1) 134 -140
3
1996
B and V photometry of the metal-rich bulge globular cluster NGC 6304
Eduardo Luiz Damiani Bica , Yazan Momany , Beatriz Barbuy , Sergio Ortolani
Astronomy and Astrophysics 357 495 -500
2000
BH 176 and AM-2: globular or open clusters?
Eduardo Luiz Damiani Bica , Beatriz Barbuy , Sergio Ortolani
Astronomy and Astrophysics 300 726
1
1995
Abundance analysis of the bulge globular clusters NGC 6553 and NGC 6528
Yazan Momany , M. Rich , Manuela Zoccali , Alvio Renzini
Memoire della Sociétà Astronomica Italiana 75 398 -399
2004
NGC 6522 : an intermediate metallicity globular cluster projected on the baade window
Eduardo Luiz Damiani Bica , Beatriz Barbuy , Sergio Ortolani
Astronomy and Astrophysics 285 ( 3) 871 -874
1994
ESO 280-SC06 : a new globular cluster in the galaxy
Eduardo Luiz Damiani Bica , Beatriz Barbuy , Sergio Ortolani
Astronomy and Astrophysics 361
2000
Ngc 6603 : a young rich open cluster towards the bulge
Eduardo Luiz Damiani Bica , Beatriz Barbuy , Sergio Ortolani
Astronomy and Astrophysics 270 117 -121
1
1993
The globular cluster NGC 6540.
Eduardo Luiz Damiani Bica , Beatriz Barbuy , Sergio Ortolani
Astronomy and Astrophysics 283 ( 1) 67 -75
1
1994
High-metallicity effects in BVRI colour-magnitude diagrams : the globular cluster NGC 6553
Eduardo Luiz Damiani Bica , Beatriz Barbuy , Sergio Ortolani
Astronomy and Astrophysics 236 ( 2) 362 -370
2
1990
Three globular cluster candidates in the direction of the bulge shown to be small emission nebulae
E Bica , JJ Clariá , Ch Bonatto , Andres E Piatti
Astronomy and Astrophysics 303 ( 3) 747 -752
1
1995
Blanketing effects in the very metal-rich bulge globular cluster Terzan 1.
Eduardo Luiz Damiani Bica , Beatriz Barbuy , Sergio Ortolani
Astronomy and Astrophysics 267 ( 1) 66 -74
2
1993
VLT-FLAMES Analysis of 8 giants in the Bulge Metal-poor Globular Cluster NGC 6522: Oldest Cluster in the Galaxy? ⋆ Analysis of 8 giants in NGC 6522
Eduardo Luiz Damiani Bica , Manuela Zoccali , Alvio Renzini , Beatriz Barbuy
Astronomy and Astrophysics 507 ( 1) 405 -415
75
2009
HIGH QUALITY SEEING V, I AND GUNN Z IMAGING OF TERZAN 4 : A BLUE HORIZONTAL BRANCH BULGE GLOBULAR CLUSTER
Eduardo Luiz Damiani Bica , Beatriz Barbuy , Sergio Ortolani
Astronomy and Astrophysics 319 ( 3) 850 -854
1997