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Artigo de periodico
The dissimilar chemical composition of the planet-hosting stars of the XO-2 binary system (2015)
Ramírez, I; Khanal, S; Aleo, P; Sobotka, A; Liu, F; Casagrande, L; Moreno, Jorge Luiz Meléndez; Yong, D; Lambert, D. L; Asplund, M
Source: The Astrophysical Journal. Unidade: IAG
Subjects: PLANETAS, ABUNDÂNCIA ESTELAR, ESTRELAS
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ABNT
RAMÍREZ, I et al. The dissimilar chemical composition of the planet-hosting stars of the XO-2 binary system. The Astrophysical Journal, v. 808, p. 13/1-13/14, 2015Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/808/1/13. Acesso em: 15 out. 2024.
APA
Ramírez, I., Khanal, S., Aleo, P., Sobotka, A., Liu, F., Casagrande, L., et al. (2015). The dissimilar chemical composition of the planet-hosting stars of the XO-2 binary system. The Astrophysical Journal, 808, 13/1-13/14. doi:10.1088/0004-637X/808/1/13
NLM
Ramírez I, Khanal S, Aleo P, Sobotka A, Liu F, Casagrande L, Moreno JLM, Yong D, Lambert DL, Asplund M. The dissimilar chemical composition of the planet-hosting stars of the XO-2 binary system [Internet]. The Astrophysical Journal. 2015 ; 808 13/1-13/14.[citado 2024 out. 15 ] Available from: https://doi.org/10.1088/0004-637X/808/1/13
Vancouver
Ramírez I, Khanal S, Aleo P, Sobotka A, Liu F, Casagrande L, Moreno JLM, Yong D, Lambert DL, Asplund M. The dissimilar chemical composition of the planet-hosting stars of the XO-2 binary system [Internet]. The Astrophysical Journal. 2015 ; 808 13/1-13/14.[citado 2024 out. 15 ] Available from: https://doi.org/10.1088/0004-637X/808/1/13
Artigo de periodico
18 Sco: a solar twin rich in refractory and neutron-capture elements: implications for chemical tagging (2014)
Moreno, Jorge Luiz Meléndez; Ramírez, Iván; Karakas, Amanda I
Source: The Astrophysical Journal. Unidade: IAG
Subjects: ABUNDÂNCIA ESTELAR, ESTRELAS, ABUNDÂNCIAS SOLARES
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
MORENO, Jorge Luiz Meléndez e RAMÍREZ, Iván e KARAKAS, Amanda I. 18 Sco: a solar twin rich in refractory and neutron-capture elements: implications for chemical tagging. The Astrophysical Journal, v. 791, p. 14/1-14/14, 2014Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/791/1/14. Acesso em: 15 out. 2024.
APA
Moreno, J. L. M., Ramírez, I., & Karakas, A. I. (2014). 18 Sco: a solar twin rich in refractory and neutron-capture elements: implications for chemical tagging. The Astrophysical Journal, 791, 14/1-14/14. doi:10.1088/0004-637X/791/1/14
NLM
Moreno JLM, Ramírez I, Karakas AI. 18 Sco: a solar twin rich in refractory and neutron-capture elements: implications for chemical tagging [Internet]. The Astrophysical Journal. 2014 ; 791 14/1-14/14.[citado 2024 out. 15 ] Available from: https://doi.org/10.1088/0004-637X/791/1/14
Vancouver
Moreno JLM, Ramírez I, Karakas AI. 18 Sco: a solar twin rich in refractory and neutron-capture elements: implications for chemical tagging [Internet]. The Astrophysical Journal. 2014 ; 791 14/1-14/14.[citado 2024 out. 15 ] Available from: https://doi.org/10.1088/0004-637X/791/1/14
Artigo de periodico
Stellar chemical abundances: in pursuit of the highest achievable precision (2014)
Bedell, Megan; Moreno, Jorge Luiz Meléndez; Bean, Jacob L; Ramírez, Ivan; Leite, Paulo; Asplund, Martin
Source: The Astrophysical Journal. Unidade: IAG
Subjects: ESTRELAS, ABUNDÂNCIA ESTELAR, ESPECTROSCOPIA
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
BEDELL, Megan et al. Stellar chemical abundances: in pursuit of the highest achievable precision. The Astrophysical Journal, v. 795, p. 23/1-23/14, 2014Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/795/1/23. Acesso em: 15 out. 2024.
APA
Bedell, M., Moreno, J. L. M., Bean, J. L., Ramírez, I., Leite, P., & Asplund, M. (2014). Stellar chemical abundances: in pursuit of the highest achievable precision. The Astrophysical Journal, 795, 23/1-23/14. doi:10.1088/0004-637X/795/1/23
NLM
Bedell M, Moreno JLM, Bean JL, Ramírez I, Leite P, Asplund M. Stellar chemical abundances: in pursuit of the highest achievable precision [Internet]. The Astrophysical Journal. 2014 ; 795 23/1-23/14.[citado 2024 out. 15 ] Available from: https://doi.org/10.1088/0004-637X/795/1/23
Vancouver
Bedell M, Moreno JLM, Bean JL, Ramírez I, Leite P, Asplund M. Stellar chemical abundances: in pursuit of the highest achievable precision [Internet]. The Astrophysical Journal. 2014 ; 795 23/1-23/14.[citado 2024 out. 15 ] Available from: https://doi.org/10.1088/0004-637X/795/1/23
Artigo de periodico
Oxygen abundances in low- and high-'alfa' field halo stars and the discovery of two field stars born in globular clusters (2012)
Ramírez, I; Meléndez Moreno, Jorge Luis; Chanamé, J
Source: The Astrophysical Journal. Unidade: IAG
Subjects: FORMAÇÃO E EVOLUÇÃO DA GALÁXIA, ABUNDÂNCIA ESTELAR, POPULAÇÕES ESTELARES
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
RAMÍREZ, I e MELÉNDEZ MORENO, Jorge Luis e CHANAMÉ, J. Oxygen abundances in low- and high-'alfa' field halo stars and the discovery of two field stars born in globular clusters. The Astrophysical Journal, v. 757, p. 164/1-164/13, 2012Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/757/2/164. Acesso em: 15 out. 2024.
APA
Ramírez, I., Meléndez Moreno, J. L., & Chanamé, J. (2012). Oxygen abundances in low- and high-'alfa' field halo stars and the discovery of two field stars born in globular clusters. The Astrophysical Journal, 757, 164/1-164/13. doi:10.1088/0004-637X/757/2/164
NLM
Ramírez I, Meléndez Moreno JL, Chanamé J. Oxygen abundances in low- and high-'alfa' field halo stars and the discovery of two field stars born in globular clusters [Internet]. The Astrophysical Journal. 2012 ; 757 164/1-164/13.[citado 2024 out. 15 ] Available from: https://doi.org/10.1088/0004-637X/757/2/164
Vancouver
Ramírez I, Meléndez Moreno JL, Chanamé J. Oxygen abundances in low- and high-'alfa' field halo stars and the discovery of two field stars born in globular clusters [Internet]. The Astrophysical Journal. 2012 ; 757 164/1-164/13.[citado 2024 out. 15 ] Available from: https://doi.org/10.1088/0004-637X/757/2/164
Artigo de periodico
Elemental abundance differences in the 16 Cygni binary system: a signature of gas giant planet formation? (2011)
Ramírez, I; Meléndez Moreno, Jorge Luis; Cornejo, D; Roederer, I. U; Fish, J. R
Source: The Astrophysical Journal. Unidade: IAG
Subjects: PLANETAS, ABUNDÂNCIA ESTELAR, ESTRELAS
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
RAMÍREZ, I et al. Elemental abundance differences in the 16 Cygni binary system: a signature of gas giant planet formation?. The Astrophysical Journal, v. 740, p. 76/1-76/15, 2011Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/740/2/76. Acesso em: 15 out. 2024.
APA
Ramírez, I., Meléndez Moreno, J. L., Cornejo, D., Roederer, I. U., & Fish, J. R. (2011). Elemental abundance differences in the 16 Cygni binary system: a signature of gas giant planet formation? The Astrophysical Journal, 740, 76/1-76/15. doi:10.1088/0004-637X/740/2/76
NLM
Ramírez I, Meléndez Moreno JL, Cornejo D, Roederer IU, Fish JR. Elemental abundance differences in the 16 Cygni binary system: a signature of gas giant planet formation? [Internet]. The Astrophysical Journal. 2011 ; 740 76/1-76/15.[citado 2024 out. 15 ] Available from: https://doi.org/10.1088/0004-637X/740/2/76
Vancouver
Ramírez I, Meléndez Moreno JL, Cornejo D, Roederer IU, Fish JR. Elemental abundance differences in the 16 Cygni binary system: a signature of gas giant planet formation? [Internet]. The Astrophysical Journal. 2011 ; 740 76/1-76/15.[citado 2024 out. 15 ] Available from: https://doi.org/10.1088/0004-637X/740/2/76

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