Zobrazeno 1 - 10
of 54
pro vyhledávání: '"Maria Bergemann"'
Autor:
Ekaterina Magg, Maria Bergemann, Aldo Serenelli, Manuel Bautista, Bertrand Plez, Ulrike Heiter, Jeffrey M. Gerber, Hans-Günter Ludwig, Sarbani Basu, Jason W. Ferguson, Helena Carvajal Gallego, Sébastien Gamrath, Patrick Palmeri, Pascal Quinet
Publikováno v:
Magg, E, Bergemann, M, Serenelli, A, Bautista, M, Plez, B, Heiter, U, Gerber, J M, Ludwig, H, Basu, S, Ferguson, J W, Gallego, H C, Gamrath, S, Palmeri, P & Quinet, P 2022, ' Observational constraints on the origin of the elements : IV. Standard composition of the Sun ', Astronomy & Astrophysics, vol. 661, A140 . https://doi.org/10.1051/0004-6361/202142971
The chemical composition of the Sun is requested in the context of various studies in astrophysics, among them in the calculation of the standard solar models (SSMs), which describe the evolution of the Sun from the pre-main-sequence to its present a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1edcb72b1068f67d61785a884671a517
http://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-476105
http://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-476105
Autor:
Denis Mourard, Maria Bergemann, Luca Casagrande, Kevin Belkacem, Regner Trampedach, Nicolas Nardetto, Daniel R. Reese, Carlos del Burgo, Marie-Jo Goupil, Victor Silva Aguirre, Andrea Chiavassa, Thierry Morel, Matthew Raymond Gent, Bertrand Plez, Douglas J. Marshall, Martin Asplund, Maria Tsantaki, Jonay I. González Hernández, Aldo Serenelli, Mikhail Kovalev, Luisa Fernanda Rodríguez Díaz, Lionel Bigot, Ulrike Heiter, Vardan Adibekyan, Szabolcs Mészáros, Jeffrey M. Gerber, Rhita-Maria Ouazzani, Thibault Merle
Publikováno v:
Gent, M R, Bergemann, M, Serenelli, A, Casagrande, L, Gerber, J M, Heiter, U, Kovalev, M, Morel, T, Nardetto, N, Adibekyan, V, Aguirre, V S, Asplund, M, Belkacem, K, Del Burgo, C, Bigot, L, Chiavassa, A, Rodríguez Díaz, L F, Goupil, M J, Hernández, J I G, Mourard, D, Merle, T, Mészáros, S, Marshall, D J, Ouazzani, R M, Plez, B, Reese, D, Trampedach, R & Tsantaki, M 2022, ' The SAPP pipeline for the determination of stellar abundances and atmospheric parameters of stars in the core program of the PLATO mission ', Astronomy and Astrophysics, vol. 658, A147 . https://doi.org/10.1051/0004-6361/202140863
Raymond, M, Bergemann, M, Serenelli, A M, Casagrande, L, Gerber, M, Heiter, U, Kovalev, M, Morel, T, Nardetto, N, Adibekyan, V, Aguirre, V S, Asplund, M, Belkacem, K, Del Burgo, C, Bigot, L, Chiavassa, A, Díaz-Aranda, L M, Goupil, M-J, González Hernández, J, Goupil, M-J, Trampedach, R & Tsantaki, M 2022, ' The SAPP pipeline for the determination of stellar abundances and atmospheric parameters of stars in the core program of the PLATO mission ', Astonomy & astrophysics, vol. 658, A147 . https://doi.org/10.1051/0004-6361/202140863
Raymond, M, Bergemann, M, Serenelli, A M, Casagrande, L, Gerber, M, Heiter, U, Kovalev, M, Morel, T, Nardetto, N, Adibekyan, V, Aguirre, V S, Asplund, M, Belkacem, K, Del Burgo, C, Bigot, L, Chiavassa, A, Díaz-Aranda, L M, Goupil, M-J, González Hernández, J, Goupil, M-J, Trampedach, R & Tsantaki, M 2022, ' The SAPP pipeline for the determination of stellar abundances and atmospheric parameters of stars in the core program of the PLATO mission ', Astonomy & astrophysics, vol. 658, A147 . https://doi.org/10.1051/0004-6361/202140863
We introduce the SAPP (Stellar Abundances and atmospheric Parameters Pipeline), the prototype of the code that will be used to determine parameters of stars observed within the core program of the PLATO space mission. The pipeline is based on the Bay
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::18328d7ed366f06a4cd6f4a9df0d126e
http://hdl.handle.net/10261/296075
http://hdl.handle.net/10261/296075
Autor:
Paul G. Beck, M. G. Pedersen, Maria Bergemann, Vincent Van Eylen, Ignasi Ribas, Conny Aerts, Ian Czekala, Nicolas Lodieu, Eline Tolstoy, Marie Martig, Nate Bastian, Benard Nsamba, Davide Gandolfi, Ana Escorza, Keivan G. Stassun, Aldo Serenelli, George C. Angelou, Y. Lebreton, J. M. Bestenlehner, A. Moya, Krešimir Pavlovski, Achim Weiss, M. M. Miller Bertolami, J. S. G. Mombarg, D. Baroch, Victor Silva Aguirre, Diane Feuillet, Fabian Schneider, Juan Carlos Morales, Konstanze Zwintz, Mark Gieles, Nancy Elias-Rosa, Léo Girardi, Pier-Emmanuel Tremblay
Publikováno v:
The Astronomy and Astrophysics Review, 29, 1-141
The Astronomy and Astrophysics Review
Astronomy and Astrophysics Review
Astronomy and Astrophysics Review, Springer Verlag, 2021, 29 (1), pp.4. ⟨10.1007/s00159-021-00132-9⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
Serenelli, A, Weiss, A, Aerts, C, Angelou, G C, Baroch, D, Bastian, N, Beck, P G, Bergemann, M, Bestenlehner, J M, Czekala, I, Elias-Rosa, N, Escorza, A, Van Eylen, V, Feuillet, D K, Gandolfi, D, Gieles, M, Girardi, L, Lebreton, Y, Lodieu, N, Martig, M, Miller Bertolami, M M, Mombarg, J S G, Morales, J C, Moya, A, Nsamba, B, Pavlovski, K, Pedersen, M G, Ribas, I, Schneider, F R N, Silva Aguirre, V, Stassun, K G, Tolstoy, E, Tremblay, P E & Zwintz, K 2021, ' Weighing stars from birth to death : mass determination methods across the HRD ', Astronomy and Astrophysics Review, vol. 29, no. 1, 4 . https://doi.org/10.1007/s00159-021-00132-9
Astronomy and Astrophysics Review, 2021, 29 (1), pp.4. ⟨10.1007/s00159-021-00132-9⟩
The Astronomy and Astrophysics Review, 29, 1, pp. 1-141
The Astronomy and Astrophysics Review
Astronomy and Astrophysics Review
Astronomy and Astrophysics Review, Springer Verlag, 2021, 29 (1), pp.4. ⟨10.1007/s00159-021-00132-9⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
Serenelli, A, Weiss, A, Aerts, C, Angelou, G C, Baroch, D, Bastian, N, Beck, P G, Bergemann, M, Bestenlehner, J M, Czekala, I, Elias-Rosa, N, Escorza, A, Van Eylen, V, Feuillet, D K, Gandolfi, D, Gieles, M, Girardi, L, Lebreton, Y, Lodieu, N, Martig, M, Miller Bertolami, M M, Mombarg, J S G, Morales, J C, Moya, A, Nsamba, B, Pavlovski, K, Pedersen, M G, Ribas, I, Schneider, F R N, Silva Aguirre, V, Stassun, K G, Tolstoy, E, Tremblay, P E & Zwintz, K 2021, ' Weighing stars from birth to death : mass determination methods across the HRD ', Astronomy and Astrophysics Review, vol. 29, no. 1, 4 . https://doi.org/10.1007/s00159-021-00132-9
Astronomy and Astrophysics Review, 2021, 29 (1), pp.4. ⟨10.1007/s00159-021-00132-9⟩
The Astronomy and Astrophysics Review, 29, 1, pp. 1-141
The mass of a star is the most fundamental parameter for its structure, evolution, and final fate. It is particularly important for any kind of stellar archaeology and characterization of exoplanets. There exist a variety of methods in astronomy to e
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0989a27c3e883ec587ab4cf7d39bff9c
http://sedici.unlp.edu.ar/handle/10915/132501
http://sedici.unlp.edu.ar/handle/10915/132501
Autor:
Jennifer L. van Saders, Léo Girardi, Johanna Teske, Emma Willett, Dennis Stello, Tiago L. Campante, M. Vrard, William J. Chaplin, Marc H. Pinsonneault, Savita Mathur, Andreas Christ Sølvsten Jørgensen, Paul G. Beck, Andrea Miglio, Martin Bo Nielsen, B. Mosser, Aldo Serenelli, Thaíse S. Rodrigues, Rafael A. García, Maria Bergemann, Josefina Montalbán, Jamie Tayar, Oliver J. Hall, Sarbani Basu, Luca Casagrande, Domenico Nardiello, Yvonne Elsworth, Rachael L. Beaton, Saniya Khan, Warrick H. Ball, Christina Chiappini, Victor Silva Aguirre, J. Ted Mackereth, Diego Bossini
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
MNRAS
MNRAS, 2021, 502 (2), pp.1947-1966. ⟨10.1093/mnras/stab098⟩
Monthly Notices of the Royal Astronomical Society
Mackereth, J T, Miglio, A, Elsworth, Y, Mosser, B, Mathur, S, Garcia, R A, Nardiello, D, Hall, O J, Vrard, M, Ball, W H, Basu, S, Beaton, R L, Beck, P G, Bergemann, M, Bossini, D, Casagrande, L, Campante, T L, Chaplin, W J, Chiappini, C, Girardi, L, Jørgensen, A C S, Khan, S, Montalbán, J, Nielsen, M B, Pinsonneault, M H, Rodrigues, T S, Serenelli, A, Aguirre, V S, Stello, D, Tayar, J, Teske, J, Van Saders, J L & Willett, E 2021, ' Prospects for Galactic and stellar astrophysics with asteroseismology of giant stars in the TESS continuous viewing zones and beyond ', Monthly Notices of the Royal Astronomical Society, vol. 502, no. 2, pp. 1947-1966 . https://doi.org/10.1093/mnras/stab098
instname
MNRAS
MNRAS, 2021, 502 (2), pp.1947-1966. ⟨10.1093/mnras/stab098⟩
Monthly Notices of the Royal Astronomical Society
Mackereth, J T, Miglio, A, Elsworth, Y, Mosser, B, Mathur, S, Garcia, R A, Nardiello, D, Hall, O J, Vrard, M, Ball, W H, Basu, S, Beaton, R L, Beck, P G, Bergemann, M, Bossini, D, Casagrande, L, Campante, T L, Chaplin, W J, Chiappini, C, Girardi, L, Jørgensen, A C S, Khan, S, Montalbán, J, Nielsen, M B, Pinsonneault, M H, Rodrigues, T S, Serenelli, A, Aguirre, V S, Stello, D, Tayar, J, Teske, J, Van Saders, J L & Willett, E 2021, ' Prospects for Galactic and stellar astrophysics with asteroseismology of giant stars in the TESS continuous viewing zones and beyond ', Monthly Notices of the Royal Astronomical Society, vol. 502, no. 2, pp. 1947-1966 . https://doi.org/10.1093/mnras/stab098
Mackereth, J. Ted, et al.
The NASA Transiting Exoplanet Survey Satellite (NASA-TESS) mission presents a treasure trove for understanding the stars it observes and the Milky Way, in which they reside. We present a first look at the prospects for
The NASA Transiting Exoplanet Survey Satellite (NASA-TESS) mission presents a treasure trove for understanding the stars it observes and the Milky Way, in which they reside. We present a first look at the prospects for
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0835056cc075e8b8e5fa7fffb1a8891a
http://hdl.handle.net/10261/261330
http://hdl.handle.net/10261/261330
Autor:
M. Deal, Angela Bragaglia, Rodolfo Smiljanic, Amelia Bayo, Aldo Serenelli, Ekaterina Semenova, Camilla Juul Hansen, L. Morbidelli, Giovanni Carraro, A. J. Gallagher, Maria Bergemann, Elena Pancino, Thomas Bensby
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
instname
Atomic diusion and mixing processes in stellar interiors influence the structure and the surface composition of stars. Some of these processes cannot yet be modelled from the first principles, and they require calibrations. This limits their applicab
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::63f7b0843edd0ad613a3a2bd747a823a
http://hdl.handle.net/10261/234001
http://hdl.handle.net/10261/234001
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
instname
[Context] The method of gyrochronology relates the age of its star to its rotation period. However, recent evidence of deviations from gyrochronology relations has been reported in the literature.
[Aims] We study the influence of tidal interacti
[Aims] We study the influence of tidal interacti
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::80a7c9dcf97cdf33e0762dba326537eb
http://arxiv.org/abs/2009.03624
http://arxiv.org/abs/2009.03624
Autor:
M. Tsantaki, T. L. Campante, A. A. Hakobyan, J. P. Faria, Mahmoudreza Oshagh, C. Allende Prieto, A. Recio-Blanco, Nuno C. Santos, Vardan Adibekyan, S. G. Sousa, Maria Bergemann, P. Figueira, P. de Laverny, J. I. Gonzaalez Hernaandez, G. Israelian, E. Delgado Mena, T. Boule
Gaia benchmark stars are selected to be calibration stars for different spectroscopic surveys. Very high-quality and homogeneous spectroscopic data for these stars are therefore required. We collected ultrahigh-resolution ESPRESSO spectra for 30 of t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::20c1378e8e576e4fe0a9cfb3926f7148
http://arxiv.org/abs/2008.08371
http://arxiv.org/abs/2008.08371
Autor:
William J. Chaplin, Aldo M. Serenelli, Andrea Miglio, Thierry Morel, J. Ted Mackereth, Fiorenzo Vincenzo, Hans Kjeldsen, Sarbani Basu, Warrick H. Ball, Amalie Stokholm, Kuldeep Verma, Jakob Rørsted Mosumgaard, Victor Silva Aguirre, Anwesh Mazumdar, Pritesh Ranadive, H. M. Antia, Yveline Lebreton, Joel Ong, Thierry Appourchaux, Timothy R. Bedding, Jørgen Christensen-Dalsgaard, Orlagh Creevey, Rafael A. García, Rasmus Handberg, Daniel Huber, Steven D. Kawaler, Mikkel N. Lund, Travis S. Metcalfe, Keivan G. Stassun, Michäel Bazot, Paul G. Beck, Keaton J. Bell, Maria Bergemann, Derek L. Buzasi, Othman Benomar, Diego Bossini, Lisa Bugnet, Tiago L. Campante, Zeynep Çelik Orhan, Enrico Corsaro, Lucía González-Cuesta, Guy R. Davies, Maria Pia Di Mauro, Ricky Egeland, Yvonne P. Elsworth, Patrick Gaulme, Hamed Ghasemi, Zhao Guo, Oliver J. Hall, Amir Hasanzadeh, Saskia Hekker, Rachel Howe, Jon M. Jenkins, Antonio Jiménez, René Kiefer, James S. Kuszlewicz, Thomas Kallinger, David W. Latham, Mia S. Lundkvist, Savita Mathur, Josefina Montalbán, Benoit Mosser, Andres Moya Bedón, Martin Bo Nielsen, Sibel Örtel, Ben M. Rendle, George R. Ricker, Thaíse S. Rodrigues, Ian W. Roxburgh, Hossein Safari, Mathew Schofield, Sara Seager, Barry Smalley, Dennis Stello, Róbert Szabó, Jamie Tayar, Nathalie Themeßl, Alexandra E. L. Thomas, Roland K. Vanderspek, Walter E. van Rossem, Mathieu Vrard, Achim Weiss, Timothy R. White, Joshua N. Winn, Mutlu Yıldız
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
Nature Astronomy
Nature Astronomy, Nature Publishing Group, 2020, 4 (4), pp.382-389. ⟨10.1038/s41550-019-0975-9⟩
Nature Astronomy, 2020, 4 (4), pp.382-389. ⟨10.1038/s41550-019-0975-9⟩
Nature Astronomy, Nature Publishing Group, 2020, ⟨10.1038/s41550-019-0975-9⟩
Chaplin, W J, Serenelli, A M, Miglio, A, Morel, T, Mackereth, J T, Vincenzo, F, Kjeldsen, H, Basu, S, Ball, W H, Stokholm, A, Verma, K, Mosumgaard, J R, Silva Aguirre, V, Mazumdar, A, Ranadive, P, Antia, H M, Lebreton, Y, Ong, J, Appourchaux, T, Bedding, T R, Christensen-Dalsgaard, J, Creevey, O, García, R A, Handberg, R, Huber, D, Kawaler, S D, Lund, M N, Metcalfe, T S, Stassun, K G, Bazot, M, Beck, P G, Bell, K J, Bergemann, M, Buzasi, D L, Benomar, O, Bossini, D, Bugnet, L, Campante, T L, Orhan, Z Ç, Corsaro, E, González-Cuesta, L, Davies, G R, Di Mauro, M P, Egeland, R, Elsworth, Y P, Gaulme, P, Ghasemi, H, Guo, Z, Hall, O J, Hasanzadeh, A, Hekker, S, Howe, R, Jenkins, J M, Jiménez, A, Kiefer, R, Kuszlewicz, J S, Kallinger, T, Latham, D W, Lundkvist, M S, Mathur, S, Montalbán, J, Mosser, B, Bedón, A M, Nielsen, M B, Örtel, S, Rendle, B M, Ricker, G R, Rodrigues, T S, Roxburgh, I W, Safari, H, Schofield, M, Seager, S, Smalley, B, Stello, D, Szabó, R, Tayar, J, Themeßl, N, Thomas, A E L, Vanderspek, R K, van Rossem, W E, Vrard, M, Weiss, A, White, T R, Winn, J N & Yıldız, M 2020, ' Age dating of an early Milky Way merger via asteroseismology of the naked-eye star ν Indi ', Nature Astronomy, vol. 4, no. 4, pp. 382-+ . https://doi.org/10.1038/s41550-019-0975-9
instname
Nature Astronomy
Nature Astronomy, Nature Publishing Group, 2020, 4 (4), pp.382-389. ⟨10.1038/s41550-019-0975-9⟩
Nature Astronomy, 2020, 4 (4), pp.382-389. ⟨10.1038/s41550-019-0975-9⟩
Nature Astronomy, Nature Publishing Group, 2020, ⟨10.1038/s41550-019-0975-9⟩
Chaplin, W J, Serenelli, A M, Miglio, A, Morel, T, Mackereth, J T, Vincenzo, F, Kjeldsen, H, Basu, S, Ball, W H, Stokholm, A, Verma, K, Mosumgaard, J R, Silva Aguirre, V, Mazumdar, A, Ranadive, P, Antia, H M, Lebreton, Y, Ong, J, Appourchaux, T, Bedding, T R, Christensen-Dalsgaard, J, Creevey, O, García, R A, Handberg, R, Huber, D, Kawaler, S D, Lund, M N, Metcalfe, T S, Stassun, K G, Bazot, M, Beck, P G, Bell, K J, Bergemann, M, Buzasi, D L, Benomar, O, Bossini, D, Bugnet, L, Campante, T L, Orhan, Z Ç, Corsaro, E, González-Cuesta, L, Davies, G R, Di Mauro, M P, Egeland, R, Elsworth, Y P, Gaulme, P, Ghasemi, H, Guo, Z, Hall, O J, Hasanzadeh, A, Hekker, S, Howe, R, Jenkins, J M, Jiménez, A, Kiefer, R, Kuszlewicz, J S, Kallinger, T, Latham, D W, Lundkvist, M S, Mathur, S, Montalbán, J, Mosser, B, Bedón, A M, Nielsen, M B, Örtel, S, Rendle, B M, Ricker, G R, Rodrigues, T S, Roxburgh, I W, Safari, H, Schofield, M, Seager, S, Smalley, B, Stello, D, Szabó, R, Tayar, J, Themeßl, N, Thomas, A E L, Vanderspek, R K, van Rossem, W E, Vrard, M, Weiss, A, White, T R, Winn, J N & Yıldız, M 2020, ' Age dating of an early Milky Way merger via asteroseismology of the naked-eye star ν Indi ', Nature Astronomy, vol. 4, no. 4, pp. 382-+ . https://doi.org/10.1038/s41550-019-0975-9
This paper includes data collected by the TESS mission, which are publicly available from the Mikulski Archive for Space Telescopes (MAST). et al.
Over the course of its history, the Milky Way has ingested multiple smaller satellite galaxies. Al
Over the course of its history, the Milky Way has ingested multiple smaller satellite galaxies. Al
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::03ccee12f9bc030b91d40cddfdeac2a4
http://hdl.handle.net/10261/236163
http://hdl.handle.net/10261/236163
Autor:
Chris Evans, Lee Patrick, Maria Bergemann, Ben Davies, R. P. Kudritzki, Annette N. M. Ferguson
Publikováno v:
Proceedings of the International Astronomical Union. 14:213-216
Red Supergiant Stars (RSGs) are important probes of stellar and chemical evolution in star-forming environments. They represent the brightest near-IR stellar components of external galaxies and probe the most recent stellar population to provide robu
Autor:
E. Tognelli, M. Van der Swaelmen, Gerry Gilmore, G. Casali, E. Pancino, Sofia Feltzing, Ulrike Heiter, Paula Jofre, A. Bragaglia, R. Bonito, Veronica Roccatagliata, Nicoletta Sanna, Simone Zaggia, F. M. Jiménez-Esteban, Maria Bergemann, Antonio Frasca, R. J. Jackson, Scilla Degl'Innocenti, Antonella Vallenari, Christian L. Sahlholdt, P. G. Prada Moroni, E. Franciosini, Thomas Bensby, Šarūnas Mikolaitis, Loredana Prisinzano, E. Stonkute, John D. Lewis, Y. Chorniy, V. Bagdonas, L. Morbidelli, Nadège Lagarde, G. Carraro, Arnas Drazdauskas, Sofia Randich, Grazina Tautvaisiene, A. C. Lanzafame, Lorenzo Spina, G. G. Sacco, Andreas Korn, S. G. Sousa, Rodolfo Smiljanic, S. L. Martell, Francesco Damiani, Thomas Masseron, Sergey E. Koposov, R. Minkeviciute, A. Hourihane, E. Friel, R. D. Jeffries, Amelia Bayo, Laura Magrini, C. C. Worley, G. Kordopatis, Anais Gonneau
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2019, 629, pp.A62. ⟨10.1051/0004-6361/201935282⟩
Casali, G, Magrini, L, Tognelli, E, Jackson, R, Jeffries, R D, Lagarde, N, Tautvaisiene, G, Masseron, T, Degl'Innocenti, S, Moroni, P G P, Kordopatis, G, Pancino, E, Randich, S, Feltzing, S, Sahlholdt, C, Spina, L, Friel, E, Roccatagliata, V, Sanna, N, Bragaglia, A, Drazdauskas, A, Mikolaitis, S, Minkeviciute, R, Stonkute, E, Chorniy, Y, Bagdonas, V, Jimenez-Esteban, F, Martell, S, Swaelmen, M V D, Gilmore, G, Vallenari, A, Bensby, T, Koposov, S E, Korn, A, Worley, C, Smiljanic, R, Bergemann, M, Carraro, G, Damiani, F, Prisinzano, L, Bonito, R, Franciosini, E, Gonneau, A, Hourihane, A, Jofre, P, Lewis, J, Morbidelli, L, Sacco, G, Sousa, S G, Zaggia, S, Lanzafame, A C, Heiter, U, Frasca, A & Bayo, A 2019, ' The Gaia-ESO survey: Calibrating a relationship between Age and the [C/N] abundance ratio with open clusters ', Astronomy and Astrophysics . https://doi.org/10.1051/0004-6361/201935282
Astronomy and Astrophysics
Astronomy and Astrophysics-A&A, EDP Sciences, 2019, 629, pp.A62. ⟨10.1051/0004-6361/201935282⟩
Casali, G, Magrini, L, Tognelli, E, Jackson, R, Jeffries, R D, Lagarde, N, Tautvaisiene, G, Masseron, T, Degl'Innocenti, S, Moroni, P G P, Kordopatis, G, Pancino, E, Randich, S, Feltzing, S, Sahlholdt, C, Spina, L, Friel, E, Roccatagliata, V, Sanna, N, Bragaglia, A, Drazdauskas, A, Mikolaitis, S, Minkeviciute, R, Stonkute, E, Chorniy, Y, Bagdonas, V, Jimenez-Esteban, F, Martell, S, Swaelmen, M V D, Gilmore, G, Vallenari, A, Bensby, T, Koposov, S E, Korn, A, Worley, C, Smiljanic, R, Bergemann, M, Carraro, G, Damiani, F, Prisinzano, L, Bonito, R, Franciosini, E, Gonneau, A, Hourihane, A, Jofre, P, Lewis, J, Morbidelli, L, Sacco, G, Sousa, S G, Zaggia, S, Lanzafame, A C, Heiter, U, Frasca, A & Bayo, A 2019, ' The Gaia-ESO survey: Calibrating a relationship between Age and the [C/N] abundance ratio with open clusters ', Astronomy and Astrophysics . https://doi.org/10.1051/0004-6361/201935282
Astronomy and Astrophysics
In the era of large high-resolution spectroscopic surveys, high-quality spectra can contribute to our understanding of the Galactic chemical evolution, providing chemical abundances belonging to the different nucleosynthesis channels, and also provid
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::831825571a5afc8e1b4471ef0eec36bb
https://hal.archives-ouvertes.fr/hal-02418986
https://hal.archives-ouvertes.fr/hal-02418986