Zobrazeno 1 - 10
of 14
pro vyhledávání: '"K. M. Cunha"'
Autor:
H. J. Rocha-Pinto, F. Almeida-Fernandes, Hélio D Perottoni, S. R. Majewski, K. M. Cunha, Diogo Souto, Simone Daflon, J. V. Sales Silva
The close relationship between the nature of the Triangulum-Andromeda (TriAnd) overdensity and the Galactic disk has become increasingly evident in recent years. However, the chemical pattern of this overdensity (R$_{GC}$ = 20 - 30 kpc) is unique and
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3480050c1df342d52b05f4ceabab6251
http://arxiv.org/abs/2007.15764
http://arxiv.org/abs/2007.15764
Autor:
M. Nobre Pereira, K. M. Cunha, Teresa Sá Marques, Cláudia Guerreiro, Vanda Areias, Hellen Ramos
Publikováno v:
Pulmonology, Vol 27, Iss 4, Pp 375-380 (2021)
Autor:
Verne V. Smith, Antonela Monachesi, D. A. García-Hernández, Jennifer Sobeck, Rebecca Lane, S. Meszaros, Roger E. Cohen, J. G. Fernandez-Trincado, Nicolas F. Martin, Felipe Gran, Baitian Tang, Henrik Jönsson, Ricardo R. Muñoz, Beatriz Barbuy, Else Starkenburg, Doug Geisler, Lorenzo Monaco, F. Mauro, Márcio Catelan, D. González-Díaz, Joel R. Brownstein, K. M. Cunha, J. E. O'Connell, Sandro Villanova, A. Rojas-Arriagada, C. E. Ferreira Lopes, C. Muñoz, Lady Henao, Y. Reinarz, Dante Minniti, R. Contreras Ramos, Cristián E. Cortés, Javier Alonso-García, Danny Horta, C. Moni Bidin, S. R. Majewski, Manuela Zoccali, T. A. Santander, Timothy C. Beers, Celeste Parisi, A. Arentsen, R. E. Miranda
Publikováno v:
Astronomy and astrophysics, 652:A157. EDP Sciences
Context. Bulge globular clusters (BGCs) are exceptional tracers of the formation and chemodynamical evolution of this oldest Galactic component. However, until now, observational difficulties have prevented us from taking full advantage of these powe
Autor:
H. J. Rocha-Pinto, Diogo Souto, H. D. Perottoni, K. M. Cunha, F. Almeida-Fernandes, J. V. Sales Silva
Publikováno v:
Proceedings of the International Astronomical Union. 14:122-124
The outer stellar halo is home to a number of substructures that are remnants of former interactions of the Galaxy with its dwarf satellites. Triangulum-Andromeda (TriAnd) is one of these halo substructures, found as a debris cloud by Rocha-Pinto et
Autor:
Ulisses Brito, Helena G. Ramos, Tânia Marques, K. M. Cunha, Isabel Ruivo, Djamila Neves, Marta Sofia Nobre Pereira, Vanda Areias, Cláudia Guerreiro
Publikováno v:
Airway pharmacology and treatment.
Introduction: Inhaled medication is crucial for asthma, COPD and their overlap (ACO) treatment. Inhaler mishandling reduces its effect, leading to clinical and functional declining. Aim: To assess inhalation technique of patients (pts) with asthma, C
Autor:
Matthew Shetrone, Thomas Masseron, Sz. Meszaros, Roger E. Cohen, Bengt Edvardsson, Doug Geisler, K. M. Cunha, H. Jönsson, Olga Zamora, F. Dell'Agli, C. Allende Prieto, Timothy C. Beers, D. A. García-Hernández, José G. Fernández-Trincado, B. Plez
We analyze a large sample of 885 GCs giants from the APOGEE survey. We used the Cannon results to separate the red giant branch and the asymptotic giant branch stars, not only allowing for a refinement of surface gravity from isochrones, but also pro
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8757ebd97b2990483e2a61c2f072f85e
http://arxiv.org/abs/1812.08817
http://arxiv.org/abs/1812.08817
Autor:
Sten Hasselquist, Mathias Schultheis, Anna B. A. Queiroz, Dante Minniti, Manuela Zoccali, Cristina Chiappini, Gail Zasowski, T. K. Fritz, Christian Nitschelm, D. A. García-Hernández, Olga Zamora, José G. Fernández-Trincado, Ricardo R. Muñoz, K. M. Cunha, A. Rojas-Arriagada
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 642, pp.A81. ⟨10.1051/0004-6361/202038327⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 642, pp.A81. ⟨10.1051/0004-6361/202038327⟩
The Galactic Center region, including the nuclear disk, has until recently been largely avoided in chemical census studies because of extreme extinction and stellar crowding. Making use of the latest APOGEE data release (DR16), we are able for the fi
Autor:
Ulisses Brito, Jose Contreras, Vanda Areias, Fernanda Nascimento, Marta Sofia Nobre Pereira, Djamila Neves, Helena G. Ramos, Isabel Ruivo, K. M. Cunha, Cláudia Guerreiro, Bruno Santos
Publikováno v:
Clinical Problems.
Autor:
S. R. Majewski, M. Schultheis, G. Zasowski, D. V. Bizyaev, J. Brinkmann, J. A. Holtzman, B. Tang, R. Carrera, H. Jönsson, Dante Minniti, A. Roman-Lopes, K. M. Cunha, C. Nitschelm, S. Villanova, G. Nandakumar, A. Rojas-Arriagada, Doug Geisler, Timothy C. Beers, C. Allende Prieto, Michael R. Hayden, A. E. Garcia Perez, F. Hearty, Roger E. Cohen, J. G. Fernandez-Trincado, D. P. Schneider, Claudia Maraston
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2017, 600, pp.A14. ⟨10.1051/0004-6361/201630154⟩
Schultheis, M, Rojas-Arriagada, A, Pérez, A E G, Jönsson, H, Hayden, M, Nandakumar, G, Cunha, K, Prieto, C A, Holtzman, J A, Beers, T C, Bizyaev, D, Brinkmann, J, Carrera, R, Cohen, R E, Geisler, D, Hearty, F R, Fernández-Trincado, J G, Maraston, C, Minniti, D, Nitschelm, C, Roman-Lopes, A, Schneider, D P, Tang, B, Villanova, S, Zasowski, G & Majewski, S R 2017, ' Baade's window with APOGEE : metallicities, ages and chemical abundances ', Astronomy and Astrophysics, vol. 600, A14 . https://doi.org/10.1051/0004-6361/201630154
Astronomy and Astrophysics-A&A, EDP Sciences, 2017, 600, pp.A14. ⟨10.1051/0004-6361/201630154⟩
Schultheis, M, Rojas-Arriagada, A, Pérez, A E G, Jönsson, H, Hayden, M, Nandakumar, G, Cunha, K, Prieto, C A, Holtzman, J A, Beers, T C, Bizyaev, D, Brinkmann, J, Carrera, R, Cohen, R E, Geisler, D, Hearty, F R, Fernández-Trincado, J G, Maraston, C, Minniti, D, Nitschelm, C, Roman-Lopes, A, Schneider, D P, Tang, B, Villanova, S, Zasowski, G & Majewski, S R 2017, ' Baade's window with APOGEE : metallicities, ages and chemical abundances ', Astronomy and Astrophysics, vol. 600, A14 . https://doi.org/10.1051/0004-6361/201630154
Baade's window (BW) is one of the most observed Galactic bulge fields in terms of chemical abundances. Due to its low and homogeneous interstellar absorption it is considered as a calibration field for Galactic bulge studies. In the era of large spec
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8e4c3cd65a7d8e4409f84e3bb0a4cf97
http://arxiv.org/abs/1702.01547
http://arxiv.org/abs/1702.01547
Autor:
Marc H. Pinsonneault, Inese I. Ivans, D. A. García-Hernández, Matthew Shetrone, Ricardo Carrera, K. M. Cunha, Peter M. Frinchaboy, Dmitry Bizyaev, A. E. García Pérez, B. Tang, Friedrich Anders, Olga Zamora, S. R. Majewski, Jennifer Sobeck, Kaike Pan, Jo Bovy, Jon A. Holtzman, Verne V. Smith, Diogo Souto, Doug Geisler, C. Allende Prieto, Sandro Villanova, Sz. Mészáros
NGC 2420 is a $\sim$2 Gyr-old well-populated open cluster that lies about 2 kpc beyond the solar circle, in the general direction of the Galactic anti-center. Most previous abundance studies have found this cluster to be mildly metal-poor, but with a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6de1da8876b5472dcbf09f1aa9e75278