Filtros : "BARBUY, BEATRIZ LEONOR SILVEIRA" "Astrophysical Journal" Removido: "2008" Limpar

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  • Source: Astrophysical Journal. Unidade: IAG

    Subjects: ASTRONOMIA, GALÁXIAS

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    • ABNT

      ORTOLANI, S e BICA, E e BARBUY, Beatriz Leonor Silveira. AL 3 (BH 261): a new globular cluster in the galaxy. Astrophysical Journal, v. 646, p. L115-L118, 2006Tradução . . Acesso em: 30 ago. 2024.
    • APA

      Ortolani, S., Bica, E., & Barbuy, B. L. S. (2006). AL 3 (BH 261): a new globular cluster in the galaxy. Astrophysical Journal, 646, L115-L118.
    • NLM

      Ortolani S, Bica E, Barbuy BLS. AL 3 (BH 261): a new globular cluster in the galaxy. Astrophysical Journal. 2006 ; 646 L115-L118.[citado 2024 ago. 30 ]
    • Vancouver

      Ortolani S, Bica E, Barbuy BLS. AL 3 (BH 261): a new globular cluster in the galaxy. Astrophysical Journal. 2006 ; 646 L115-L118.[citado 2024 ago. 30 ]
  • Source: Astrophysical Journal. Unidade: IAG

    Subjects: GALÁXIAS, ASTROFÍSICA ESTELAR

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    • ABNT

      BURSTEIN, David et al. Globular cluster and galaxy formation: M31, the milky way, and implications for globular cluster systems of spiral galaxies. Astrophysical Journal, v. 614, p. 158-166, 2004Tradução . . Acesso em: 30 ago. 2024.
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      Burstein, D., Li, Y., Feeman, K. C., Norris, J. E., Bessell, M. S., Hawthorn, J. B., et al. (2004). Globular cluster and galaxy formation: M31, the milky way, and implications for globular cluster systems of spiral galaxies. Astrophysical Journal, 614, 158-166.
    • NLM

      Burstein D, Li Y, Feeman KC, Norris JE, Bessell MS, Hawthorn JB, Gibson BK, Beasley MA, Lee H-C, Barbuy BLS, Huchra JP, Brodie JP, Forbes DA. Globular cluster and galaxy formation: M31, the milky way, and implications for globular cluster systems of spiral galaxies. Astrophysical Journal. 2004 ;614 158-166.[citado 2024 ago. 30 ]
    • Vancouver

      Burstein D, Li Y, Feeman KC, Norris JE, Bessell MS, Hawthorn JB, Gibson BK, Beasley MA, Lee H-C, Barbuy BLS, Huchra JP, Brodie JP, Forbes DA. Globular cluster and galaxy formation: M31, the milky way, and implications for globular cluster systems of spiral galaxies. Astrophysical Journal. 2004 ;614 158-166.[citado 2024 ago. 30 ]
  • Source: Astrophysical Journal. Unidade: IAG

    Assunto: ASTROFÍSICA ESTELAR

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    • ABNT

      BARBUY, Beatriz Leonor Silveira et al. Oxygen abundance in the template halo giant HD '122563 POT.1'. Astrophysical Journal, v. 588, p. 1072-1081, 2003Tradução . . Acesso em: 30 ago. 2024.
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      Barbuy, B. L. S., Meléndez, J., Spite Monique,, Spite, F., Depagne, E., Hill, V., et al. (2003). Oxygen abundance in the template halo giant HD '122563 POT.1'. Astrophysical Journal, 588, 1072-1081.
    • NLM

      Barbuy BLS, Meléndez J, Spite Monique, Spite F, Depagne E, Hill V, Cayrel R, Bonifacio P, Damineli Neto A, Torres CAO. Oxygen abundance in the template halo giant HD '122563 POT.1'. Astrophysical Journal. 2003 ;588 1072-1081.[citado 2024 ago. 30 ]
    • Vancouver

      Barbuy BLS, Meléndez J, Spite Monique, Spite F, Depagne E, Hill V, Cayrel R, Bonifacio P, Damineli Neto A, Torres CAO. Oxygen abundance in the template halo giant HD '122563 POT.1'. Astrophysical Journal. 2003 ;588 1072-1081.[citado 2024 ago. 30 ]
  • Source: Astrophysical Journal. Unidade: IAG

    Assunto: GALÁXIAS

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    • ABNT

      POMPÉIA, Luciana e BARBUY, Beatriz Leonor Silveira e GRENON, Michel. Detailed analysis of nearby bulgelike dwarf stars. III. 'alfa'-element and heavy-element abundances. Astrophysical Journal, v. 592, p. 1173-1185, 2003Tradução . . Acesso em: 30 ago. 2024.
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      Pompéia, L., Barbuy, B. L. S., & Grenon, M. (2003). Detailed analysis of nearby bulgelike dwarf stars. III. 'alfa'-element and heavy-element abundances. Astrophysical Journal, 592, 1173-1185.
    • NLM

      Pompéia L, Barbuy BLS, Grenon M. Detailed analysis of nearby bulgelike dwarf stars. III. 'alfa'-element and heavy-element abundances. Astrophysical Journal. 2003 ; 592 1173-1185.[citado 2024 ago. 30 ]
    • Vancouver

      Pompéia L, Barbuy BLS, Grenon M. Detailed analysis of nearby bulgelike dwarf stars. III. 'alfa'-element and heavy-element abundances. Astrophysical Journal. 2003 ; 592 1173-1185.[citado 2024 ago. 30 ]
  • Source: Astrophysical Journal. Unidade: IAG

    Assunto: ASTROFÍSICA ESTELAR

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    • ABNT

      POMPÉIA, Luciana e BARBUY, Beatriz Leonor Silveira e GRENON, Michel. Detailed analysis of nearby bulgelike dwarf Stars. II. Lithium abundances. Astrophysical Journal, v. 570, p. 820-824, 2002Tradução . . Acesso em: 30 ago. 2024.
    • APA

      Pompéia, L., Barbuy, B. L. S., & Grenon, M. (2002). Detailed analysis of nearby bulgelike dwarf Stars. II. Lithium abundances. Astrophysical Journal, 570, 820-824.
    • NLM

      Pompéia L, Barbuy BLS, Grenon M. Detailed analysis of nearby bulgelike dwarf Stars. II. Lithium abundances. Astrophysical Journal. 2002 ; 570 820-824.[citado 2024 ago. 30 ]
    • Vancouver

      Pompéia L, Barbuy BLS, Grenon M. Detailed analysis of nearby bulgelike dwarf Stars. II. Lithium abundances. Astrophysical Journal. 2002 ; 570 820-824.[citado 2024 ago. 30 ]
  • Source: Astrophysical Journal. Unidade: IAG

    Assunto: ASTROFÍSICA ESTELAR

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      MELÉNDEZ, Jorge. Keck NIRSPEC Infrared OH Lines: Oxygen Abundances in Metal-poor Stars down to [Fe/H] = -2. Astrophysical Journal, v. 575, p. 474-483, 2002Tradução . . Acesso em: 30 ago. 2024.
    • APA

      Meléndez, J. (2002). Keck NIRSPEC Infrared OH Lines: Oxygen Abundances in Metal-poor Stars down to [Fe/H] = -2. Astrophysical Journal, 575, 474-483.
    • NLM

      Meléndez J. Keck NIRSPEC Infrared OH Lines: Oxygen Abundances in Metal-poor Stars down to [Fe/H] = -2. Astrophysical Journal. 2002 ; 575 474-483.[citado 2024 ago. 30 ]
    • Vancouver

      Meléndez J. Keck NIRSPEC Infrared OH Lines: Oxygen Abundances in Metal-poor Stars down to [Fe/H] = -2. Astrophysical Journal. 2002 ; 575 474-483.[citado 2024 ago. 30 ]
  • Source: Astrophysical Journal. Unidade: IAG

    Assunto: ASTROFÍSICA ESTELAR

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    • ABNT

      POMPÉIA, Luciana e BARBUY, Beatriz Leonor Silveira e GRENON, Michel. Detailed analysis of nearby bulgelike dwarf stars. I. Stellar parameters, kinematics, and oxygen abundances. Astrophysical Journal, v. 566, p. 845-856, 2002Tradução . . Acesso em: 30 ago. 2024.
    • APA

      Pompéia, L., Barbuy, B. L. S., & Grenon, M. (2002). Detailed analysis of nearby bulgelike dwarf stars. I. Stellar parameters, kinematics, and oxygen abundances. Astrophysical Journal, 566, 845-856.
    • NLM

      Pompéia L, Barbuy BLS, Grenon M. Detailed analysis of nearby bulgelike dwarf stars. I. Stellar parameters, kinematics, and oxygen abundances. Astrophysical Journal. 2002 ; 566 845-856.[citado 2024 ago. 30 ]
    • Vancouver

      Pompéia L, Barbuy BLS, Grenon M. Detailed analysis of nearby bulgelike dwarf stars. I. Stellar parameters, kinematics, and oxygen abundances. Astrophysical Journal. 2002 ; 566 845-856.[citado 2024 ago. 30 ]
  • Source: Astrophysical Journal. Unidade: IAG

    Assunto: ASTROFÍSICA ESTELAR

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    • ABNT

      MELÉNDEZ, Jorge e BARBUY, Beatriz Leonor Silveira e SPITE, François. Oxygen abundances in metal-poor stars (-2.2<[Fe/H]<-1.2) from infrared oh lines. Astrophysical Journal, v. 556, p. 858-871, 2001Tradução . . Acesso em: 30 ago. 2024.
    • APA

      Meléndez, J., Barbuy, B. L. S., & Spite, F. (2001). Oxygen abundances in metal-poor stars (-2.2<[Fe/H]<-1.2) from infrared oh lines. Astrophysical Journal, 556, 858-871.
    • NLM

      Meléndez J, Barbuy BLS, Spite F. Oxygen abundances in metal-poor stars (-2.2<[Fe/H]<-1.2) from infrared oh lines. Astrophysical Journal. 2001 ; 556 858-871.[citado 2024 ago. 30 ]
    • Vancouver

      Meléndez J, Barbuy BLS, Spite F. Oxygen abundances in metal-poor stars (-2.2<[Fe/H]<-1.2) from infrared oh lines. Astrophysical Journal. 2001 ; 556 858-871.[citado 2024 ago. 30 ]
  • Source: Astrophysical Journal. Unidade: IAG

    Subjects: ASTRONOMIA, ASTROFÍSICA ESTELAR, GALÁXIAS

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      SCHIAVON, R P e BARBUY, Beatriz Leonor Silveira e BRUZUAL, A G. Near-infrared spectral features in single-aged stellar populations. Astrophysical Journal, v. 532, n. 1 pt. 1, p. 453-460, 2000Tradução . . Acesso em: 30 ago. 2024.
    • APA

      Schiavon, R. P., Barbuy, B. L. S., & Bruzual, A. G. (2000). Near-infrared spectral features in single-aged stellar populations. Astrophysical Journal, 532( 1 pt. 1), 453-460.
    • NLM

      Schiavon RP, Barbuy BLS, Bruzual AG. Near-infrared spectral features in single-aged stellar populations. Astrophysical Journal. 2000 ; 532( 1 pt. 1): 453-460.[citado 2024 ago. 30 ]
    • Vancouver

      Schiavon RP, Barbuy BLS, Bruzual AG. Near-infrared spectral features in single-aged stellar populations. Astrophysical Journal. 2000 ; 532( 1 pt. 1): 453-460.[citado 2024 ago. 30 ]
  • Source: Astrophysical Journal. Unidade: IAG

    Subjects: ASTRONOMIA, ASTROFÍSICA ESTELAR

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      SCHIAVON, Ricardo Piorno e BARBUY, Beatriz Leonor Silveira. The temperature scale of metal-rich M giants based on TiO bands: population synthesis in the near-infrared. Astrophysical Journal, v. 510, n. 2 pt.1, p. L934-L943, 1999Tradução . . Acesso em: 30 ago. 2024.
    • APA

      Schiavon, R. P., & Barbuy, B. L. S. (1999). The temperature scale of metal-rich M giants based on TiO bands: population synthesis in the near-infrared. Astrophysical Journal, 510( 2 pt.1), L934-L943.
    • NLM

      Schiavon RP, Barbuy BLS. The temperature scale of metal-rich M giants based on TiO bands: population synthesis in the near-infrared. Astrophysical Journal. 1999 ; 510( 2 pt.1): L934-L943.[citado 2024 ago. 30 ]
    • Vancouver

      Schiavon RP, Barbuy BLS. The temperature scale of metal-rich M giants based on TiO bands: population synthesis in the near-infrared. Astrophysical Journal. 1999 ; 510( 2 pt.1): L934-L943.[citado 2024 ago. 30 ]
  • Source: Astrophysical Journal. Unidade: IAG

    Subjects: ASTRONOMIA, ASTROFÍSICA ESTELAR

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      SCHIAVON, Ricardo Piorno et al. The near-infrared Na'iota'doublet feature in M stars. Astrophysical Journal, v. 479, n. 2, p. 902-906, 1997Tradução . . Acesso em: 30 ago. 2024.
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      Schiavon, R. P., Barbuy, B. L. S., Rossi, S. C. F., & Milone, A. de C. (1997). The near-infrared Na'iota'doublet feature in M stars. Astrophysical Journal, 479( 2), 902-906.
    • NLM

      Schiavon RP, Barbuy BLS, Rossi SCF, Milone A de C. The near-infrared Na'iota'doublet feature in M stars. Astrophysical Journal. 1997 ; 479( 2): 902-906.[citado 2024 ago. 30 ]
    • Vancouver

      Schiavon RP, Barbuy BLS, Rossi SCF, Milone A de C. The near-infrared Na'iota'doublet feature in M stars. Astrophysical Journal. 1997 ; 479( 2): 902-906.[citado 2024 ago. 30 ]
  • Source: Astrophysical Journal. Unidade: IAG

    Subjects: ASTRONOMIA, AGLOMERADOS DE GALÁXIAS, GALÁXIAS

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    • ABNT

      BICA, Eduardo et al. Capture of field stars by globular clusters in dense bulge regions. Astrophysical Journal, v. 482, n. ju 1997, p. L49-L51, 1997Tradução . . Acesso em: 30 ago. 2024.
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      Bica, E., Dottori, H., Oliveira Filho, I. R., Ortolani, S., & Barbuy, B. L. S. (1997). Capture of field stars by globular clusters in dense bulge regions. Astrophysical Journal, 482( ju 1997), L49-L51.
    • NLM

      Bica E, Dottori H, Oliveira Filho IR, Ortolani S, Barbuy BLS. Capture of field stars by globular clusters in dense bulge regions. Astrophysical Journal. 1997 ; 482( ju 1997): L49-L51.[citado 2024 ago. 30 ]
    • Vancouver

      Bica E, Dottori H, Oliveira Filho IR, Ortolani S, Barbuy BLS. Capture of field stars by globular clusters in dense bulge regions. Astrophysical Journal. 1997 ; 482( ju 1997): L49-L51.[citado 2024 ago. 30 ]
  • Source: Astrophysical Journal. Unidade: IAG

    Subjects: ASTRONOMIA, ASTROFÍSICA ESTELAR, ESTRELAS

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    • ABNT

      SCHIAVON, Ricardo Piorno e BARBUY, Beatriz Leonor Silveira e SINGH, Patan Deen. The FeH Wing-Ford band in spectra of M stars. Astrophysical Journal, v. 484, n. 1, p. 499-510, 1997Tradução . . Acesso em: 30 ago. 2024.
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      Schiavon, R. P., Barbuy, B. L. S., & Singh, P. D. (1997). The FeH Wing-Ford band in spectra of M stars. Astrophysical Journal, 484( 1), 499-510.
    • NLM

      Schiavon RP, Barbuy BLS, Singh PD. The FeH Wing-Ford band in spectra of M stars. Astrophysical Journal. 1997 ; 484( 1): 499-510.[citado 2024 ago. 30 ]
    • Vancouver

      Schiavon RP, Barbuy BLS, Singh PD. The FeH Wing-Ford band in spectra of M stars. Astrophysical Journal. 1997 ; 484( 1): 499-510.[citado 2024 ago. 30 ]
  • Source: Astrophysical Journal. Unidade: IAG

    Subjects: ASTRONOMIA, ASTROQUÍMICA, ASTROFÍSICA ESTELAR

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      SILVA, L. e REZA, R e BARBUY, Beatriz Leonor Silveira. Carbon isotope ratios in very lithium-rich k giants. Astrophysical Journal, v. 448, n. 1 pt. 2, p. l41-144, 1995Tradução . . Acesso em: 30 ago. 2024.
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      Silva, L., Reza, R., & Barbuy, B. L. S. (1995). Carbon isotope ratios in very lithium-rich k giants. Astrophysical Journal, 448( 1 pt. 2), l41-144.
    • NLM

      Silva L, Reza R, Barbuy BLS. Carbon isotope ratios in very lithium-rich k giants. Astrophysical Journal. 1995 ; 448( 1 pt. 2): l41-144.[citado 2024 ago. 30 ]
    • Vancouver

      Silva L, Reza R, Barbuy BLS. Carbon isotope ratios in very lithium-rich k giants. Astrophysical Journal. 1995 ; 448( 1 pt. 2): l41-144.[citado 2024 ago. 30 ]
  • Source: Astrophysical Journal. Unidade: IAG

    Subjects: ASTRONOMIA, GALÁXIAS

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      BARBUY, Beatriz Leonor Silveira. Calibration of 'MG IND.2' versus ['FE' / h] and ['MG' / 'FE']. Astrophysical Journal, v. 430, n. 1 pt. 1, p. 218-221, 1994Tradução . . Acesso em: 30 ago. 2024.
    • APA

      Barbuy, B. L. S. (1994). Calibration of 'MG IND.2' versus ['FE' / h] and ['MG' / 'FE']. Astrophysical Journal, 430( 1 pt. 1), 218-221.
    • NLM

      Barbuy BLS. Calibration of 'MG IND.2' versus ['FE' / h] and ['MG' / 'FE']. Astrophysical Journal. 1994 ; 430( 1 pt. 1): 218-221.[citado 2024 ago. 30 ]
    • Vancouver

      Barbuy BLS. Calibration of 'MG IND.2' versus ['FE' / h] and ['MG' / 'FE']. Astrophysical Journal. 1994 ; 430( 1 pt. 1): 218-221.[citado 2024 ago. 30 ]
  • Source: Astrophysical Journal. Unidade: IAG

    Assunto: ASTRONOMIA

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      BICA, E e BARBUY, Beatriz Leonor Silveira e ORTOLANI, S. Metal-righ giant branches of bulge clusters: application to color-magnitude diagrams of m31 and m32. Astrophysical Journal, v. 382, p. l15-117, 1991Tradução . . Acesso em: 30 ago. 2024.
    • APA

      Bica, E., Barbuy, B. L. S., & Ortolani, S. (1991). Metal-righ giant branches of bulge clusters: application to color-magnitude diagrams of m31 and m32. Astrophysical Journal, 382, l15-117.
    • NLM

      Bica E, Barbuy BLS, Ortolani S. Metal-righ giant branches of bulge clusters: application to color-magnitude diagrams of m31 and m32. Astrophysical Journal. 1991 ; 382 l15-117.[citado 2024 ago. 30 ]
    • Vancouver

      Bica E, Barbuy BLS, Ortolani S. Metal-righ giant branches of bulge clusters: application to color-magnitude diagrams of m31 and m32. Astrophysical Journal. 1991 ; 382 l15-117.[citado 2024 ago. 30 ]

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