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Artigo de periodico
X-ray and star formation: ROSAT observations of the Monoceros and Rosette molecular clouds (1998)
Gregório-Hetem, Jane; Montmerle, T; Casanova, S; Feigelson, E D
Source: Astronomy and Astrophysics. Unidade: IAG
Subjects: ASTRONOMIA, ASTROFÍSICA ESTELAR, RAIOS X
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ABNT
GREGÓRIO-HETEM, Jane et al. X-ray and star formation: ROSAT observations of the Monoceros and Rosette molecular clouds. Astronomy and Astrophysics, v. 331, n. 1, p. 193-210, 1998Tradução . . Acesso em: 19 abr. 2024.
APA
Gregório-Hetem, J., Montmerle, T., Casanova, S., & Feigelson, E. D. (1998). X-ray and star formation: ROSAT observations of the Monoceros and Rosette molecular clouds. Astronomy and Astrophysics, 331( 1), 193-210.
NLM
Gregório-Hetem J, Montmerle T, Casanova S, Feigelson ED. X-ray and star formation: ROSAT observations of the Monoceros and Rosette molecular clouds. Astronomy and Astrophysics. 1998 ; 331( 1): 193-210.[citado 2024 abr. 19 ]
Vancouver
Gregório-Hetem J, Montmerle T, Casanova S, Feigelson ED. X-ray and star formation: ROSAT observations of the Monoceros and Rosette molecular clouds. Astronomy and Astrophysics. 1998 ; 331( 1): 193-210.[citado 2024 abr. 19 ]
Artigo de periodico
What drives the Balmer extinction sequence in spiral galaxies?: Clus from the sloan digital sky Survey (2004)
Stasinska, G; Mateus Júnior, Abílio; Sodré Júnior, Laerte; Szczerba, R
Source: Astronomy and Astrophysics. Unidade: IAG
Assunto: GALÁXIAS
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STASINSKA, G et al. What drives the Balmer extinction sequence in spiral galaxies?: Clus from the sloan digital sky Survey. Astronomy and Astrophysics, v. 420, p. 475-489, 2004Tradução . . Acesso em: 19 abr. 2024.
APA
Stasinska, G., Mateus Júnior, A., Sodré Júnior, L., & Szczerba, R. (2004). What drives the Balmer extinction sequence in spiral galaxies?: Clus from the sloan digital sky Survey. Astronomy and Astrophysics, 420, 475-489.
NLM
Stasinska G, Mateus Júnior A, Sodré Júnior L, Szczerba R. What drives the Balmer extinction sequence in spiral galaxies?: Clus from the sloan digital sky Survey. Astronomy and Astrophysics. 2004 ;420 475-489.[citado 2024 abr. 19 ]
Vancouver
Stasinska G, Mateus Júnior A, Sodré Júnior L, Szczerba R. What drives the Balmer extinction sequence in spiral galaxies?: Clus from the sloan digital sky Survey. Astronomy and Astrophysics. 2004 ;420 475-489.[citado 2024 abr. 19 ]
Artigo de periodico
Variability and pulsations in the Be star 66 Ophiuchi (2002)
Floquet, M; Neiner, C; Janot-Pacheco, Eduardo; Hubert, A M; Jankov, S; Zorec, J; Briot, D; Chauville, J; Leister, Nelson Vani; Percy, J R; Ballereau, D; Bakos, A G
Source: Astronomy and Astrophysics. Unidade: IAG
Assunto: ASTROFÍSICA ESTELAR
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FLOQUET, M et al. Variability and pulsations in the Be star 66 Ophiuchi. Astronomy and Astrophysics, v. 394, p. 137-149, 2002Tradução . . Disponível em: https://doi.org/10.1051/0004-6361:20021105. Acesso em: 19 abr. 2024.
APA
Floquet, M., Neiner, C., Janot-Pacheco, E., Hubert, A. M., Jankov, S., Zorec, J., et al. (2002). Variability and pulsations in the Be star 66 Ophiuchi. Astronomy and Astrophysics, 394, 137-149. doi:10.1051/0004-6361:20021105
NLM
Floquet M, Neiner C, Janot-Pacheco E, Hubert AM, Jankov S, Zorec J, Briot D, Chauville J, Leister NV, Percy JR, Ballereau D, Bakos AG. Variability and pulsations in the Be star 66 Ophiuchi [Internet]. Astronomy and Astrophysics. 2002 ;394 137-149.[citado 2024 abr. 19 ] Available from: https://doi.org/10.1051/0004-6361:20021105
Vancouver
Floquet M, Neiner C, Janot-Pacheco E, Hubert AM, Jankov S, Zorec J, Briot D, Chauville J, Leister NV, Percy JR, Ballereau D, Bakos AG. Variability and pulsations in the Be star 66 Ophiuchi [Internet]. Astronomy and Astrophysics. 2002 ;394 137-149.[citado 2024 abr. 19 ] Available from: https://doi.org/10.1051/0004-6361:20021105
Artigo de periodico
VLT-UVES spectroscopy of a bulge giant magnified through microlensing: EROS-BLG-2000-5 (2002)
Minniti, D; Barbuy, Beatriz Leonor Silveira; Hill, V; Bica; Ortolani, S; Rich, R M; Cook, K H; Vandehei, T; Renzini, A; Pasquini, L; Bennett, D
Source: Astronomy and Astrophysics. Unidade: IAG
Assunto: ASTROFÍSICA ESTELAR
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MINNITI, D et al. VLT-UVES spectroscopy of a bulge giant magnified through microlensing: EROS-BLG-2000-5. Astronomy and Astrophysics, v. 384, p. 884-889, 2002Tradução . . Disponível em: https://doi.org/10.1051/0004-6361:20020111. Acesso em: 19 abr. 2024.
APA
Minniti, D., Barbuy, B. L. S., Hill, V., Bica,, Ortolani, S., Rich, R. M., et al. (2002). VLT-UVES spectroscopy of a bulge giant magnified through microlensing: EROS-BLG-2000-5. Astronomy and Astrophysics, 384, 884-889. doi:10.1051/0004-6361:20020111
NLM
Minniti D, Barbuy BLS, Hill V, Bica, Ortolani S, Rich RM, Cook KH, Vandehei T, Renzini A, Pasquini L, Bennett D. VLT-UVES spectroscopy of a bulge giant magnified through microlensing: EROS-BLG-2000-5 [Internet]. Astronomy and Astrophysics. 2002 ; 384 884-889.[citado 2024 abr. 19 ] Available from: https://doi.org/10.1051/0004-6361:20020111
Vancouver
Minniti D, Barbuy BLS, Hill V, Bica, Ortolani S, Rich RM, Cook KH, Vandehei T, Renzini A, Pasquini L, Bennett D. VLT-UVES spectroscopy of a bulge giant magnified through microlensing: EROS-BLG-2000-5 [Internet]. Astronomy and Astrophysics. 2002 ; 384 884-889.[citado 2024 abr. 19 ] Available from: https://doi.org/10.1051/0004-6361:20020111
Artigo de periodico
VLT-UVES analysis of two giants in the bulge metal-poor globular cluster HP-1: analysis of two giants in HP-1 (2006)
Barbuy, Beatriz Leonor Silveira; Zoccali, M; Ortolani, S; Momany, Y; Minniti, D; Hill, V; Renzini, A; Rich, R. M; Bica, E; Pasquini, L; Yadav, K. S
Source: Astronomy and Astrophysics. Unidade: IAG
Subjects: GALÁXIAS, ESTRELAS
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ABNT
BARBUY, Beatriz Leonor Silveira et al. VLT-UVES analysis of two giants in the bulge metal-poor globular cluster HP-1: analysis of two giants in HP-1. Astronomy and Astrophysics, v. 449, p. 349-358, 2006Tradução . . Acesso em: 19 abr. 2024.
APA
Barbuy, B. L. S., Zoccali, M., Ortolani, S., Momany, Y., Minniti, D., Hill, V., et al. (2006). VLT-UVES analysis of two giants in the bulge metal-poor globular cluster HP-1: analysis of two giants in HP-1. Astronomy and Astrophysics, 449, 349-358.
NLM
Barbuy BLS, Zoccali M, Ortolani S, Momany Y, Minniti D, Hill V, Renzini A, Rich RM, Bica E, Pasquini L, Yadav KS. VLT-UVES analysis of two giants in the bulge metal-poor globular cluster HP-1: analysis of two giants in HP-1. Astronomy and Astrophysics. 2006 ; 449 349-358.[citado 2024 abr. 19 ]
Vancouver
Barbuy BLS, Zoccali M, Ortolani S, Momany Y, Minniti D, Hill V, Renzini A, Rich RM, Bica E, Pasquini L, Yadav KS. VLT-UVES analysis of two giants in the bulge metal-poor globular cluster HP-1: analysis of two giants in HP-1. Astronomy and Astrophysics. 2006 ; 449 349-358.[citado 2024 abr. 19 ]
Artigo de periodico
VLT-UVES analysis of 5 giants in 47 Tucanae (2005)
Alves-Brito, Alan; Barbuy, Beatriz Leonor Silveira; Ortolani, S; Momany, Y; Hill, V; Zoccali, M; Renzini, A; Minniti, D; Pasquini, L; Bica, E; Rich, R M
Source: Astronomy and Astrophysics. Unidade: IAG
Subjects: ASTROFÍSICA ESTELAR, ABUNDÂNCIA ESTELAR
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ALVES-BRITO, Alan et al. VLT-UVES analysis of 5 giants in 47 Tucanae. Astronomy and Astrophysics, v. 435, p. 657-667, 2005Tradução . . Disponível em: https://doi.org/10.1051/0004-6361:20041634. Acesso em: 19 abr. 2024.
APA
Alves-Brito, A., Barbuy, B. L. S., Ortolani, S., Momany, Y., Hill, V., Zoccali, M., et al. (2005). VLT-UVES analysis of 5 giants in 47 Tucanae. Astronomy and Astrophysics, 435, 657-667. doi:10.1051/0004-6361:20041634
NLM
Alves-Brito A, Barbuy BLS, Ortolani S, Momany Y, Hill V, Zoccali M, Renzini A, Minniti D, Pasquini L, Bica E, Rich RM. VLT-UVES analysis of 5 giants in 47 Tucanae [Internet]. Astronomy and Astrophysics. 2005 ; 435 657-667.[citado 2024 abr. 19 ] Available from: https://doi.org/10.1051/0004-6361:20041634
Vancouver
Alves-Brito A, Barbuy BLS, Ortolani S, Momany Y, Hill V, Zoccali M, Renzini A, Minniti D, Pasquini L, Bica E, Rich RM. VLT-UVES analysis of 5 giants in 47 Tucanae [Internet]. Astronomy and Astrophysics. 2005 ; 435 657-667.[citado 2024 abr. 19 ] Available from: https://doi.org/10.1051/0004-6361:20041634
Artigo de periodico
VLT-UVES abundance analysis of four giants in NGC 6553 (2006)
Brito, A. Alves; Barbuy, Beatriz Leonor Silveira; Zoccali, M; Minniti, D; Ortolani, S; Hill, V; Renzini, A; Pasquini, L; Bica, E; Rich, R. M; Meléndez, J; Momany, Y
Source: Astronomy and Astrophysics. Unidade: IAG
Subjects: ASTROFÍSICA ESTELAR, GALÁXIAS
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ABNT
BRITO, A. Alves et al. VLT-UVES abundance analysis of four giants in NGC 6553. Astronomy and Astrophysics, v. 460, p. 269-276, 2006Tradução . . Disponível em: https://doi.org/10.1051/0004-6361:20065488. Acesso em: 19 abr. 2024.
APA
Brito, A. A., Barbuy, B. L. S., Zoccali, M., Minniti, D., Ortolani, S., Hill, V., et al. (2006). VLT-UVES abundance analysis of four giants in NGC 6553. Astronomy and Astrophysics, 460, 269-276. doi:10.1051/0004-6361:20065488
NLM
Brito AA, Barbuy BLS, Zoccali M, Minniti D, Ortolani S, Hill V, Renzini A, Pasquini L, Bica E, Rich RM, Meléndez J, Momany Y. VLT-UVES abundance analysis of four giants in NGC 6553 [Internet]. Astronomy and Astrophysics. 2006 ; 460 269-276.[citado 2024 abr. 19 ] Available from: https://doi.org/10.1051/0004-6361:20065488
Vancouver
Brito AA, Barbuy BLS, Zoccali M, Minniti D, Ortolani S, Hill V, Renzini A, Pasquini L, Bica E, Rich RM, Meléndez J, Momany Y. VLT-UVES abundance analysis of four giants in NGC 6553 [Internet]. Astronomy and Astrophysics. 2006 ; 460 269-276.[citado 2024 abr. 19 ] Available from: https://doi.org/10.1051/0004-6361:20065488
Artigo de periodico
VLT observations of turnoff stars in the globular cluster NGC 6397 (2001)
Thévenin, F; Charbonnel, C; Freitas Pacheco, José Antonio; Idiart, Thais Eunice Pires; Jasniewicz, G; Laverny, P de; Plez, B
Source: Astronomy and Astrophysics. Unidade: IAG
Assunto: ASTROFÍSICA ESTELAR
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THÉVENIN, F et al. VLT observations of turnoff stars in the globular cluster NGC 6397. Astronomy and Astrophysics, v. 373, p. 905-915, 2001Tradução . . Disponível em: https://doi.org/10.1051/0004-6361:20010672. Acesso em: 19 abr. 2024.
APA
Thévenin, F., Charbonnel, C., Freitas Pacheco, J. A., Idiart, T. E. P., Jasniewicz, G., Laverny, P. de, & Plez, B. (2001). VLT observations of turnoff stars in the globular cluster NGC 6397. Astronomy and Astrophysics, 373, 905-915. doi:10.1051/0004-6361:20010672
NLM
Thévenin F, Charbonnel C, Freitas Pacheco JA, Idiart TEP, Jasniewicz G, Laverny P de, Plez B. VLT observations of turnoff stars in the globular cluster NGC 6397 [Internet]. Astronomy and Astrophysics. 2001 ;373 905-915.[citado 2024 abr. 19 ] Available from: https://doi.org/10.1051/0004-6361:20010672
Vancouver
Thévenin F, Charbonnel C, Freitas Pacheco JA, Idiart TEP, Jasniewicz G, Laverny P de, Plez B. VLT observations of turnoff stars in the globular cluster NGC 6397 [Internet]. Astronomy and Astrophysics. 2001 ;373 905-915.[citado 2024 abr. 19 ] Available from: https://doi.org/10.1051/0004-6361:20010672
Artigo de periodico
V,J, H and K imaging of the metal rich globular cluster NGC 6528* (2003)
Momany, Y; Ortolani, S; Held, E.V; Barbuy, Beatriz Leonor Silveira; Bica, E; Renzini, A; Bedin, L.R; Rich, R.M; Marconi, G
Source: Astronomy and Astrophysics. Unidade: IAG
Assunto: ASTROFÍSICA ESTELAR
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MOMANY, Y et al. V,J, H and K imaging of the metal rich globular cluster NGC 6528*. Astronomy and Astrophysics, v. 402, p. 607-616, 2003Tradução . . Acesso em: 19 abr. 2024.
APA
Momany, Y., Ortolani, S., Held, E. V., Barbuy, B. L. S., Bica, E., Renzini, A., et al. (2003). V,J, H and K imaging of the metal rich globular cluster NGC 6528*. Astronomy and Astrophysics, 402, 607-616.
NLM
Momany Y, Ortolani S, Held EV, Barbuy BLS, Bica E, Renzini A, Bedin LR, Rich RM, Marconi G. V,J, H and K imaging of the metal rich globular cluster NGC 6528*. Astronomy and Astrophysics. 2003 ;402 607-616.[citado 2024 abr. 19 ]
Vancouver
Momany Y, Ortolani S, Held EV, Barbuy BLS, Bica E, Renzini A, Bedin LR, Rich RM, Marconi G. V,J, H and K imaging of the metal rich globular cluster NGC 6528*. Astronomy and Astrophysics. 2003 ;402 607-616.[citado 2024 abr. 19 ]
Artigo de periodico
V, I photometry of the metal-rich bulge globular cluster Terzan 2 (1997)
Ortolani, S; Bica, E; Barbuy, Beatriz Leonor Silveira
Source: Astronomy and Astrophysics. Unidade: IAG
Subjects: ASTRONOMIA, ESTRELAS
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ORTOLANI, S e BICA, E e BARBUY, Beatriz Leonor Silveira. V, I photometry of the metal-rich bulge globular cluster Terzan 2. Astronomy and Astrophysics, v. 326, n. 2, p. 614-619, 1997Tradução . . Acesso em: 19 abr. 2024.
APA
Ortolani, S., Bica, E., & Barbuy, B. L. S. (1997). V, I photometry of the metal-rich bulge globular cluster Terzan 2. Astronomy and Astrophysics, 326( 2), 614-619.
NLM
Ortolani S, Bica E, Barbuy BLS. V, I photometry of the metal-rich bulge globular cluster Terzan 2. Astronomy and Astrophysics. 1997 ; 326( 2): 614-619.[citado 2024 abr. 19 ]
Vancouver
Ortolani S, Bica E, Barbuy BLS. V, I photometry of the metal-rich bulge globular cluster Terzan 2. Astronomy and Astrophysics. 1997 ; 326( 2): 614-619.[citado 2024 abr. 19 ]
Artigo de periodico
Using cepheids to determine the galactic abundance gradient (2002)
Andrievsky, S M; Bersier, D; Kovtyukh, V V; Luck, R E; Maciel, Walter Junqueira; Lépine, Jacques Raymond Daniel; Beletsky, Yu V
Source: Astronomy and Astrophysics. Unidade: IAG
Assunto: GALÁXIAS
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ABNT
ANDRIEVSKY, S M et al. Using cepheids to determine the galactic abundance gradient. Astronomy and Astrophysics, v. 384, p. 140-144, 2002Tradução . . Disponível em: https://doi.org/10.1051/0004-6361:20011488. Acesso em: 19 abr. 2024.
APA
Andrievsky, S. M., Bersier, D., Kovtyukh, V. V., Luck, R. E., Maciel, W. J., Lépine, J. R. D., & Beletsky, Y. V. (2002). Using cepheids to determine the galactic abundance gradient. Astronomy and Astrophysics, 384, 140-144. doi:10.1051/0004-6361:20011488
NLM
Andrievsky SM, Bersier D, Kovtyukh VV, Luck RE, Maciel WJ, Lépine JRD, Beletsky YV. Using cepheids to determine the galactic abundance gradient [Internet]. Astronomy and Astrophysics. 2002 ;384 140-144.[citado 2024 abr. 19 ] Available from: https://doi.org/10.1051/0004-6361:20011488
Vancouver
Andrievsky SM, Bersier D, Kovtyukh VV, Luck RE, Maciel WJ, Lépine JRD, Beletsky YV. Using cepheids to determine the galactic abundance gradient [Internet]. Astronomy and Astrophysics. 2002 ;384 140-144.[citado 2024 abr. 19 ] Available from: https://doi.org/10.1051/0004-6361:20011488
Artigo de periodico
Using Cepheids to determine the galactic abundance gradient: III. Firt results for the outer disc (2002)
Andrievsky, A M; Kovtyukh, V V; Luck, R E; Lépine, Jacques Raymond Daniel; Maciel, Walter Junqueira; Beletsky, Yu. V.
Source: Astronomy and Astrophysics. Unidade: IAG
Assunto: ASTROFÍSICA ESTELAR
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ANDRIEVSKY, A M et al. Using Cepheids to determine the galactic abundance gradient: III. Firt results for the outer disc. Astronomy and Astrophysics, v. 392, p. 491-499, 2002Tradução . . Acesso em: 19 abr. 2024.
APA
Andrievsky, A. M., Kovtyukh, V. V., Luck, R. E., Lépine, J. R. D., Maciel, W. J., & Beletsky, Y. V. (2002). Using Cepheids to determine the galactic abundance gradient: III. Firt results for the outer disc. Astronomy and Astrophysics, 392, 491-499.
NLM
Andrievsky AM, Kovtyukh VV, Luck RE, Lépine JRD, Maciel WJ, Beletsky YV. Using Cepheids to determine the galactic abundance gradient: III. Firt results for the outer disc. Astronomy and Astrophysics. 2002 ;392 491-499.[citado 2024 abr. 19 ]
Vancouver
Andrievsky AM, Kovtyukh VV, Luck RE, Lépine JRD, Maciel WJ, Beletsky YV. Using Cepheids to determine the galactic abundance gradient: III. Firt results for the outer disc. Astronomy and Astrophysics. 2002 ;392 491-499.[citado 2024 abr. 19 ]
Artigo de periodico
Using Cepheids to determine the galactic abundance gradient: I. the solar neighbourhood (2002)
Andrievsky, A M; Kovtyukh, V V; Luck, R E; Lépine, Jacques Raymond Daniel; Bersier, D; Maciel, Walter Junqueira; Barbuy, Beatriz Leonor Silveira; Klochkova, V G; Panchuk, V E; Karpischek, R U
Source: Astronomy and Astrophysics. Unidade: IAG
Assunto: ASTROFÍSICA ESTELAR
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ANDRIEVSKY, A M et al. Using Cepheids to determine the galactic abundance gradient: I. the solar neighbourhood. Astronomy and Astrophysics, v. 381, p. 32-50, 2002Tradução . . Acesso em: 19 abr. 2024.
APA
Andrievsky, A. M., Kovtyukh, V. V., Luck, R. E., Lépine, J. R. D., Bersier, D., Maciel, W. J., et al. (2002). Using Cepheids to determine the galactic abundance gradient: I. the solar neighbourhood. Astronomy and Astrophysics, 381, 32-50.
NLM
Andrievsky AM, Kovtyukh VV, Luck RE, Lépine JRD, Bersier D, Maciel WJ, Barbuy BLS, Klochkova VG, Panchuk VE, Karpischek RU. Using Cepheids to determine the galactic abundance gradient: I. the solar neighbourhood. Astronomy and Astrophysics. 2002 ;381 32-50.[citado 2024 abr. 19 ]
Vancouver
Andrievsky AM, Kovtyukh VV, Luck RE, Lépine JRD, Bersier D, Maciel WJ, Barbuy BLS, Klochkova VG, Panchuk VE, Karpischek RU. Using Cepheids to determine the galactic abundance gradient: I. the solar neighbourhood. Astronomy and Astrophysics. 2002 ;381 32-50.[citado 2024 abr. 19 ]
Artigo de periodico
Type i planetary nebulae in the large magellanic cloud: oxygen, sulphur and argon abundances as tracers of chemical enrichment (1993)
Freitas Pacheco, José Antonio; Barbuy, Beatriz Leonor Silveira; Costa, Roberto Dell'Aglio Dias da; Idiart, T E P
Source: Astronomy and Astrophysics. Unidade: IAG
Subjects: ASTRONOMIA, GALÁXIAS
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ABNT
FREITAS PACHECO, José Antonio et al. Type i planetary nebulae in the large magellanic cloud: oxygen, sulphur and argon abundances as tracers of chemical enrichment. Astronomy and Astrophysics, v. 271, n. 2, p. 429-434, 1993Tradução . . Acesso em: 19 abr. 2024.
APA
Freitas Pacheco, J. A., Barbuy, B. L. S., Costa, R. D. 'A. D. da, & Idiart, T. E. P. (1993). Type i planetary nebulae in the large magellanic cloud: oxygen, sulphur and argon abundances as tracers of chemical enrichment. Astronomy and Astrophysics, 271( 2), 429-434.
NLM
Freitas Pacheco JA, Barbuy BLS, Costa RD'AD da, Idiart TEP. Type i planetary nebulae in the large magellanic cloud: oxygen, sulphur and argon abundances as tracers of chemical enrichment. Astronomy and Astrophysics. 1993 ; 271( 2): 429-434.[citado 2024 abr. 19 ]
Vancouver
Freitas Pacheco JA, Barbuy BLS, Costa RD'AD da, Idiart TEP. Type i planetary nebulae in the large magellanic cloud: oxygen, sulphur and argon abundances as tracers of chemical enrichment. Astronomy and Astrophysics. 1993 ; 271( 2): 429-434.[citado 2024 abr. 19 ]
Artigo de periodico
Two reddened globular clusters projected close to the galactic center: palomar 6 and djorgovski 1 (1995)
Ortolani, S; Bica, E; Barbuy, Beatriz Leonor Silveira
Source: Astronomy and Astrophysics. Unidade: IAG
Subjects: ASTRONOMIA, ASTROFÍSICA ESTELAR
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ABNT
ORTOLANI, S e BICA, E e BARBUY, Beatriz Leonor Silveira. Two reddened globular clusters projected close to the galactic center: palomar 6 and djorgovski 1. Astronomy and Astrophysics, v. 296, n. 3, p. 680-684, 1995Tradução . . Acesso em: 19 abr. 2024.
APA
Ortolani, S., Bica, E., & Barbuy, B. L. S. (1995). Two reddened globular clusters projected close to the galactic center: palomar 6 and djorgovski 1. Astronomy and Astrophysics, 296( 3), 680-684.
NLM
Ortolani S, Bica E, Barbuy BLS. Two reddened globular clusters projected close to the galactic center: palomar 6 and djorgovski 1. Astronomy and Astrophysics. 1995 ; 296( 3): 680-684.[citado 2024 abr. 19 ]
Vancouver
Ortolani S, Bica E, Barbuy BLS. Two reddened globular clusters projected close to the galactic center: palomar 6 and djorgovski 1. Astronomy and Astrophysics. 1995 ; 296( 3): 680-684.[citado 2024 abr. 19 ]
Artigo de periodico
Triple structure in the 8km s-1 water maser source in orion (1988)
Vilas Boas, J W S; Abraham, Zulema
Source: Astronomy and Astrophysics. Unidade: IAG
Assunto: ASTRONOMIA
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VILAS BOAS, J W S e ABRAHAM, Zulema. Triple structure in the 8km s-1 water maser source in orion. Astronomy and Astrophysics, v. 204, n. 1 , p. 239-41, 1988Tradução . . Acesso em: 19 abr. 2024.
APA
Vilas Boas, J. W. S., & Abraham, Z. (1988). Triple structure in the 8km s-1 water maser source in orion. Astronomy and Astrophysics, 204( 1 ), 239-41.
NLM
Vilas Boas JWS, Abraham Z. Triple structure in the 8km s-1 water maser source in orion. Astronomy and Astrophysics. 1988 ;204( 1 ): 239-41.[citado 2024 abr. 19 ]
Vancouver
Vilas Boas JWS, Abraham Z. Triple structure in the 8km s-1 water maser source in orion. Astronomy and Astrophysics. 1988 ;204( 1 ): 239-41.[citado 2024 abr. 19 ]
Artigo de periodico
Time variations of the narrow Fe II and H I spectral emission lines from the close vicinity of 'eta' Carinae during the spectral event of 2003 (2005)
Hartman, Henrik; Damineli Neto, Augusto; Johansson, S; Letokhov, V. S
Source: Astronomy and Astrophysics. Unidade: IAG
Assunto: ASTROFÍSICA ESTELAR
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ABNT
HARTMAN, Henrik et al. Time variations of the narrow Fe II and H I spectral emission lines from the close vicinity of 'eta' Carinae during the spectral event of 2003. Astronomy and Astrophysics, v. 436, p. 945-952, 2005Tradução . . Disponível em: https://doi.org/10.1051/0004-6361:20052835. Acesso em: 19 abr. 2024.
APA
Hartman, H., Damineli Neto, A., Johansson, S., & Letokhov, V. S. (2005). Time variations of the narrow Fe II and H I spectral emission lines from the close vicinity of 'eta' Carinae during the spectral event of 2003. Astronomy and Astrophysics, 436, 945-952. doi:10.1051/0004-6361:20052835
NLM
Hartman H, Damineli Neto A, Johansson S, Letokhov VS. Time variations of the narrow Fe II and H I spectral emission lines from the close vicinity of 'eta' Carinae during the spectral event of 2003 [Internet]. Astronomy and Astrophysics. 2005 ; 436 945-952.[citado 2024 abr. 19 ] Available from: https://doi.org/10.1051/0004-6361:20052835
Vancouver
Hartman H, Damineli Neto A, Johansson S, Letokhov VS. Time variations of the narrow Fe II and H I spectral emission lines from the close vicinity of 'eta' Carinae during the spectral event of 2003 [Internet]. Astronomy and Astrophysics. 2005 ; 436 945-952.[citado 2024 abr. 19 ] Available from: https://doi.org/10.1051/0004-6361:20052835
Artigo de periodico
Time variation of the 'H IND.2'0 and sio masers in late-type stars (1986)
Gomez Balboa, A M; Lépine, Jacques Raymond Daniel
Source: Astronomy and Astrophysics. Unidade: IAG
Assunto: ASTRONOMIA
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
GOMEZ BALBOA, A M e LÉPINE, Jacques Raymond Daniel. Time variation of the 'H IND.2'0 and sio masers in late-type stars. Astronomy and Astrophysics, v. 159, p. 166-74, 1986Tradução . . Acesso em: 19 abr. 2024.
APA
Gomez Balboa, A. M., & Lépine, J. R. D. (1986). Time variation of the 'H IND.2'0 and sio masers in late-type stars. Astronomy and Astrophysics, 159, 166-74.
NLM
Gomez Balboa AM, Lépine JRD. Time variation of the 'H IND.2'0 and sio masers in late-type stars. Astronomy and Astrophysics. 1986 ;159 166-74.[citado 2024 abr. 19 ]
Vancouver
Gomez Balboa AM, Lépine JRD. Time variation of the 'H IND.2'0 and sio masers in late-type stars. Astronomy and Astrophysics. 1986 ;159 166-74.[citado 2024 abr. 19 ]
Artigo de periodico
Time variation of radial gradients in the galactic disk: electron temperatures and abundances (2007)
Maciel, Walter Junqueira; Quireza, C; Costa, Roberto Dell'Aglio Dias da
Source: Astronomy and Astrophysics. Unidade: IAG
Subjects: GALÁXIAS (EVOLUÇÃO), ABUNDÂNCIAS (ASTRONOMIA), MEIO INTERGALÁTICO
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
MACIEL, Walter Junqueira e QUIREZA, C e COSTA, Roberto Dell'Aglio Dias da. Time variation of radial gradients in the galactic disk: electron temperatures and abundances. Astronomy and Astrophysics, v. 463, n. 2, p. L13-L16, 2007Tradução . . Disponível em: https://doi.org/10.1051/0004-6361:20066916. Acesso em: 19 abr. 2024.
APA
Maciel, W. J., Quireza, C., & Costa, R. D. 'A. D. da. (2007). Time variation of radial gradients in the galactic disk: electron temperatures and abundances. Astronomy and Astrophysics, 463( 2), L13-L16. doi:10.1051/0004-6361:20066916
NLM
Maciel WJ, Quireza C, Costa RD'AD da. Time variation of radial gradients in the galactic disk: electron temperatures and abundances [Internet]. Astronomy and Astrophysics. 2007 ; 463( 2): L13-L16.[citado 2024 abr. 19 ] Available from: https://doi.org/10.1051/0004-6361:20066916
Vancouver
Maciel WJ, Quireza C, Costa RD'AD da. Time variation of radial gradients in the galactic disk: electron temperatures and abundances [Internet]. Astronomy and Astrophysics. 2007 ; 463( 2): L13-L16.[citado 2024 abr. 19 ] Available from: https://doi.org/10.1051/0004-6361:20066916
Artigo de periodico
Three globular cluster candidates in the direction of the bulge shown to be small emission nebulae (1995)
Bica, E; Claria, J J; Bonatto, C H; Piatti, A E; Ortolani, S; Barbuy, Beatriz Leonor Silveira
Source: Astronomy and Astrophysics. Unidade: IAG
Subjects: ASTRONOMIA, GALÁXIAS
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
BICA, E et al. Three globular cluster candidates in the direction of the bulge shown to be small emission nebulae. Astronomy and Astrophysics, v. no 1995, n. 3, p. 747-752, 1995Tradução . . Acesso em: 19 abr. 2024.
APA
Bica, E., Claria, J. J., Bonatto, C. H., Piatti, A. E., Ortolani, S., & Barbuy, B. L. S. (1995). Three globular cluster candidates in the direction of the bulge shown to be small emission nebulae. Astronomy and Astrophysics, no 1995( 3), 747-752.
NLM
Bica E, Claria JJ, Bonatto CH, Piatti AE, Ortolani S, Barbuy BLS. Three globular cluster candidates in the direction of the bulge shown to be small emission nebulae. Astronomy and Astrophysics. 1995 ; no 1995( 3): 747-752.[citado 2024 abr. 19 ]
Vancouver
Bica E, Claria JJ, Bonatto CH, Piatti AE, Ortolani S, Barbuy BLS. Three globular cluster candidates in the direction of the bulge shown to be small emission nebulae. Astronomy and Astrophysics. 1995 ; no 1995( 3): 747-752.[citado 2024 abr. 19 ]

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