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Artigo de periodico
Evidences of extragalactic origin and planet engulfment in the metal-poor twin pair HD 134439/HD 134440 (2018)
Reggiani, Henrique; Moreno, Jorge Luis Meléndez
Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG
Subjects: ABUNDÂNCIA ESTELAR, GALÁXIAS
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ABNT
REGGIANI, Henrique e MORENO, Jorge Luis Meléndez. Evidences of extragalactic origin and planet engulfment in the metal-poor twin pair HD 134439/HD 134440. Monthly Notices of the Royal Astronomical Society, v. 475, n. 3, p. 3502-3510, 2018Tradução . . Disponível em: https://doi.org/10.1093/mnras/sty104. Acesso em: 08 ago. 2024.
APA
Reggiani, H., & Moreno, J. L. M. (2018). Evidences of extragalactic origin and planet engulfment in the metal-poor twin pair HD 134439/HD 134440. Monthly Notices of the Royal Astronomical Society, 475( 3), 3502-3510. doi:10.1093/mnras/sty104
NLM
Reggiani H, Moreno JLM. Evidences of extragalactic origin and planet engulfment in the metal-poor twin pair HD 134439/HD 134440 [Internet]. Monthly Notices of the Royal Astronomical Society. 2018 ; 475( 3): 3502-3510.[citado 2024 ago. 08 ] Available from: https://doi.org/10.1093/mnras/sty104
Vancouver
Reggiani H, Moreno JLM. Evidences of extragalactic origin and planet engulfment in the metal-poor twin pair HD 134439/HD 134440 [Internet]. Monthly Notices of the Royal Astronomical Society. 2018 ; 475( 3): 3502-3510.[citado 2024 ago. 08 ] Available from: https://doi.org/10.1093/mnras/sty104
Artigo de periodico
Sc and neutron-capture abundances in Galactic low- and high-α field halo stars (2017)
Fishlock, C. K; Yong, D; Karakas, A. I; Alves-Brito, A; Moreno, Jorge Luiz Meléndez; Nissen, P E; Kobayashi, C; Casey, R
Source: MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. Unidade: IAG
Subjects: ABUNDÂNCIA ESTELAR, GALÁXIAS
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ABNT
FISHLOCK, C. K et al. Sc and neutron-capture abundances in Galactic low- and high-α field halo stars. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, v. 466, p. 4672-4682, 2017Tradução . . Disponível em: https://doi.org/10.1093/mnras/stx047. Acesso em: 08 ago. 2024.
APA
Fishlock, C. K., Yong, D., Karakas, A. I., Alves-Brito, A., Moreno, J. L. M., Nissen, P. E., et al. (2017). Sc and neutron-capture abundances in Galactic low- and high-α field halo stars. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 466, 4672-4682. doi:10.1093/mnras/stx047
NLM
Fishlock CK, Yong D, Karakas AI, Alves-Brito A, Moreno JLM, Nissen PE, Kobayashi C, Casey R. Sc and neutron-capture abundances in Galactic low- and high-α field halo stars [Internet]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 2017 ;466 4672-4682.[citado 2024 ago. 08 ] Available from: https://doi.org/10.1093/mnras/stx047
Vancouver
Fishlock CK, Yong D, Karakas AI, Alves-Brito A, Moreno JLM, Nissen PE, Kobayashi C, Casey R. Sc and neutron-capture abundances in Galactic low- and high-α field halo stars [Internet]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 2017 ;466 4672-4682.[citado 2024 ago. 08 ] Available from: https://doi.org/10.1093/mnras/stx047
Artigo de periodico
Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars - VI Age and abundances structure of the stellar populations in the central sub-kpc of the milky way *,** (2017)
Bensby, T; Moreno, Jorge Luis Meléndez
Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: GALÁXIAS, ABUNDÂNCIA ESTELAR
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ABNT
BENSBY, T e MORENO, Jorge Luis Meléndez. Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars - VI Age and abundances structure of the stellar populations in the central sub-kpc of the milky way *,**. Astronomy & Astrophysics, v. 605, p. 89, 2017Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201730560. Acesso em: 08 ago. 2024.
APA
Bensby, T., & Moreno, J. L. M. (2017). Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars - VI Age and abundances structure of the stellar populations in the central sub-kpc of the milky way *,**. Astronomy & Astrophysics, 605, 89. doi:10.1051/0004-6361/201730560
NLM
Bensby T, Moreno JLM. Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars - VI Age and abundances structure of the stellar populations in the central sub-kpc of the milky way *,** [Internet]. Astronomy & Astrophysics. 2017 ; 605 89.[citado 2024 ago. 08 ] Available from: https://doi.org/10.1051/0004-6361/201730560
Vancouver
Bensby T, Moreno JLM. Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars - VI Age and abundances structure of the stellar populations in the central sub-kpc of the milky way *,** [Internet]. Astronomy & Astrophysics. 2017 ; 605 89.[citado 2024 ago. 08 ] Available from: https://doi.org/10.1051/0004-6361/201730560
Artigo de periodico
G64-12 and G64-37 are carbon-enhanced metal-poor stars (2016)
Placco, Vinicius M; Beers, Timothy C; Reggiani, Henrique; Moreno, Jorge Luis Meléndez
Source: The Astrophysical Journal Letters. Unidade: IAG
Subjects: GALÁXIAS, ABUNDÂNCIA ESTELAR
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ABNT
PLACCO, Vinicius M et al. G64-12 and G64-37 are carbon-enhanced metal-poor stars. The Astrophysical Journal Letters, 2016Tradução . . Disponível em: http://iopscience.iop.org/article/10.3847/2041-8205/829/2/L24/pdf. Acesso em: 08 ago. 2024.
APA
Placco, V. M., Beers, T. C., Reggiani, H., & Moreno, J. L. M. (2016). G64-12 and G64-37 are carbon-enhanced metal-poor stars. The Astrophysical Journal Letters. doi:10.3847/2041-8205/829/2/L24
NLM
Placco VM, Beers TC, Reggiani H, Moreno JLM. G64-12 and G64-37 are carbon-enhanced metal-poor stars [Internet]. The Astrophysical Journal Letters. 2016 ;[citado 2024 ago. 08 ] Available from: http://iopscience.iop.org/article/10.3847/2041-8205/829/2/L24/pdf
Vancouver
Placco VM, Beers TC, Reggiani H, Moreno JLM. G64-12 and G64-37 are carbon-enhanced metal-poor stars [Internet]. The Astrophysical Journal Letters. 2016 ;[citado 2024 ago. 08 ] Available from: http://iopscience.iop.org/article/10.3847/2041-8205/829/2/L24/pdf
Artigo de periodico
Spatially unassociated galaxies contribute significantly to the blended submillimetre galaxy population: predictions for follow-up observations of ALMA sources (2013)
Hayward, Christopher C; Behroozi, Peter S; Somerville, Rachel S; Primack, Joel R; Moreno, Jorge Luiz Meléndez; Wechsler, Risa H
Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG
Subjects: GALÁXIAS, ABUNDÂNCIAS (ASTRONOMIA), COSMOLOGIA, ESTRUTURA DO UNIVERSO
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ABNT
HAYWARD, Christopher C et al. Spatially unassociated galaxies contribute significantly to the blended submillimetre galaxy population: predictions for follow-up observations of ALMA sources. Monthly Notices of the Royal Astronomical Society, v. 434, p. 2572-2581, 2013Tradução . . Disponível em: https://doi.org/10.1093/mnras/stt1202. Acesso em: 08 ago. 2024.
APA
Hayward, C. C., Behroozi, P. S., Somerville, R. S., Primack, J. R., Moreno, J. L. M., & Wechsler, R. H. (2013). Spatially unassociated galaxies contribute significantly to the blended submillimetre galaxy population: predictions for follow-up observations of ALMA sources. Monthly Notices of the Royal Astronomical Society, 434, 2572-2581. doi:10.1093/mnras/stt1202
NLM
Hayward CC, Behroozi PS, Somerville RS, Primack JR, Moreno JLM, Wechsler RH. Spatially unassociated galaxies contribute significantly to the blended submillimetre galaxy population: predictions for follow-up observations of ALMA sources [Internet]. Monthly Notices of the Royal Astronomical Society. 2013 ; 434 2572-2581.[citado 2024 ago. 08 ] Available from: https://doi.org/10.1093/mnras/stt1202
Vancouver
Hayward CC, Behroozi PS, Somerville RS, Primack JR, Moreno JLM, Wechsler RH. Spatially unassociated galaxies contribute significantly to the blended submillimetre galaxy population: predictions for follow-up observations of ALMA sources [Internet]. Monthly Notices of the Royal Astronomical Society. 2013 ; 434 2572-2581.[citado 2024 ago. 08 ] Available from: https://doi.org/10.1093/mnras/stt1202
Artigo de periodico
High precision differential abundance measurements in globular clusters: chemical inhomogeneities in NGC 6752 (2013)
Yong, David; Moreno, Jorge Luiz Meléndez; Grundahl, Frank; Roederer, Ian U; Norris, John E; Milone, A. P; Marino, A. F; Coelho, P; McArthur, Barbara E; Lind, K; Collet, R; Asplund, Martin
Source: Monthly Notices of The Royal Astronomical Society. Unidade: IAG
Subjects: ABUNDÂNCIA ESTELAR, GALÁXIAS
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ABNT
YONG, David et al. High precision differential abundance measurements in globular clusters: chemical inhomogeneities in NGC 6752. Monthly Notices of The Royal Astronomical Society, v. 434, p. 3542-3565, 2013Tradução . . Disponível em: https://doi.org/10.1093/mnras/stt1276. Acesso em: 08 ago. 2024.
APA
Yong, D., Moreno, J. L. M., Grundahl, F., Roederer, I. U., Norris, J. E., Milone, A. P., et al. (2013). High precision differential abundance measurements in globular clusters: chemical inhomogeneities in NGC 6752. Monthly Notices of The Royal Astronomical Society, 434, 3542-3565. doi:10.1093/mnras/stt1276
NLM
Yong D, Moreno JLM, Grundahl F, Roederer IU, Norris JE, Milone AP, Marino AF, Coelho P, McArthur BE, Lind K, Collet R, Asplund M. High precision differential abundance measurements in globular clusters: chemical inhomogeneities in NGC 6752 [Internet]. Monthly Notices of The Royal Astronomical Society. 2013 ; 434 3542-3565.[citado 2024 ago. 08 ] Available from: https://doi.org/10.1093/mnras/stt1276
Vancouver
Yong D, Moreno JLM, Grundahl F, Roederer IU, Norris JE, Milone AP, Marino AF, Coelho P, McArthur BE, Lind K, Collet R, Asplund M. High precision differential abundance measurements in globular clusters: chemical inhomogeneities in NGC 6752 [Internet]. Monthly Notices of The Royal Astronomical Society. 2013 ; 434 3542-3565.[citado 2024 ago. 08 ] Available from: https://doi.org/10.1093/mnras/stt1276
Texto na web
International team on Keck Observatory strengthens Big Bang theory. [Depoimento a Karin Lind e Davide De Martin] (2013)
Moreno, Jorge Luiz Meléndez
Unidade: IAG
Subjects: NOTÍCIA, GALÁXIA (VIA LÁCTEA), LÍTIO, GALÁXIAS
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ABNT
MORENO, Jorge Luiz Meléndez. International team on Keck Observatory strengthens Big Bang theory. [Depoimento a Karin Lind e Davide De Martin]. . Mauna Kea: W. M. Keck Observatory. Disponível em: http://www.keckobservatory.org/recent/entry/international_team_on_keck_observatory_strengthens_big_bang_theory. Acesso em: 08 ago. 2024. , 2013
APA
Moreno, J. L. M. (2013). International team on Keck Observatory strengthens Big Bang theory. [Depoimento a Karin Lind e Davide De Martin]. Mauna Kea: W. M. Keck Observatory. Recuperado de http://www.keckobservatory.org/recent/entry/international_team_on_keck_observatory_strengthens_big_bang_theory
NLM
Moreno JLM. International team on Keck Observatory strengthens Big Bang theory. [Depoimento a Karin Lind e Davide De Martin] [Internet]. 2013 ;[citado 2024 ago. 08 ] Available from: http://www.keckobservatory.org/recent/entry/international_team_on_keck_observatory_strengthens_big_bang_theory
Vancouver
Moreno JLM. International team on Keck Observatory strengthens Big Bang theory. [Depoimento a Karin Lind e Davide De Martin] [Internet]. 2013 ;[citado 2024 ago. 08 ] Available from: http://www.keckobservatory.org/recent/entry/international_team_on_keck_observatory_strengthens_big_bang_theory
Artigo de periodico
CNO and F abundances in the globular cluster M22 (NGC 6656) (2012)
Alves-Brito, A; Yong, D; Meléndez Moreno, Jorge Luis; Vásquez, S; Karakas, A. I
Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: GALÁXIAS, ABUNDÂNCIAS (ASTRONOMIA), ABUNDÂNCIA ESTELAR
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ABNT
ALVES-BRITO, A et al. CNO and F abundances in the globular cluster M22 (NGC 6656). Astronomy & Astrophysics, v. 540, p. A3/1-A3/12, 2012Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201118623. Acesso em: 08 ago. 2024.
APA
Alves-Brito, A., Yong, D., Meléndez Moreno, J. L., Vásquez, S., & Karakas, A. I. (2012). CNO and F abundances in the globular cluster M22 (NGC 6656). Astronomy & Astrophysics, 540, A3/1-A3/12. doi:10.1051/0004-6361/201118623
NLM
Alves-Brito A, Yong D, Meléndez Moreno JL, Vásquez S, Karakas AI. CNO and F abundances in the globular cluster M22 (NGC 6656) [Internet]. Astronomy & Astrophysics. 2012 ; 540 A3/1-A3/12.[citado 2024 ago. 08 ] Available from: https://doi.org/10.1051/0004-6361/201118623
Vancouver
Alves-Brito A, Yong D, Meléndez Moreno JL, Vásquez S, Karakas AI. CNO and F abundances in the globular cluster M22 (NGC 6656) [Internet]. Astronomy & Astrophysics. 2012 ; 540 A3/1-A3/12.[citado 2024 ago. 08 ] Available from: https://doi.org/10.1051/0004-6361/201118623

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