Zobrazeno 1 - 10
of 15
pro vyhledávání: '"Marilia Carlos"'
Autor:
Giacomo Cordoni, Antonino P. Milone, Anna F. Marino, Enrico Vesperini, Emanuele Dondoglio, Maria Vittoria Legnardi, Anjana Mohandasan, Marilia Carlos, Edoardo P. Lagioia, Sohee Jang, Tuila Ziliotto
Binary stars play a crucial role in our understanding of the formation and evolution of star clusters and their stellar populations. We use Gaia Data Release 3 to homogeneously analyze 78 Galactic open clusters and the unresolved binary systems they
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f3e484a6088b3057625a4d962546eca2
Publikováno v:
Repositório Institucional da USP (Biblioteca Digital da Produção Intelectual)
Universidade de São Paulo (USP)
instacron:USP
Universidade de São Paulo (USP)
instacron:USP
We determine lithium (Li) abundances for solar twins in the M67 open cluster to add valuable information about the correlation between Li depletion and stellar age and, then, better understand stellar structure and evolution. We use high resolution a
Autor:
Parth Sharma, Jorge Melendez, Marilia Carlos, Lorenzo Spina, Andrew R. Casey, Megan Bedell, Antonella Vallenari, E. Franciosini
Stellar members of binary systems are formed from the same material, therefore they should be chemically identical. However, recent high-precision studies have unveiled chemical differences between the two members of binary pairs composed by Sun-like
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::992da989013b2daff67c60e677fb372d
http://arxiv.org/abs/2108.12040
http://arxiv.org/abs/2108.12040
Autor:
Adriana Valio, Henrique Reggiani, Jorge Melendez, Jhon Yana Galarza, Diego Lorenzo-Oliveira, Lorenzo Spina, Raphaëlle D. Haywood, Marilia Carlos, Geisa Ponte, Davide Gandolfi
Publikováno v:
Repositório Institucional da USP (Biblioteca Digital da Produção Intelectual)
Universidade de São Paulo (USP)
instacron:USP
Universidade de São Paulo (USP)
instacron:USP
Spectroscopic equilibrium allows us to obtain precise stellar parameters in Sun-like stars. It relies on the assumption of the iron excitation and ionization equilibrium. However, several works suggest that magnetic activity may affect chemical abund
Autor:
Tailo Marco, Antonino P. Milone, Edoardo P. Lagioia, Francesca D'Antona, Sohee Jang, Enrico Vesperini, Anna F. Marino, Paolo Ventura, Vittoria Caloi, Marilia Carlos, Giacomo Cordoni, Emanuele Dondoglio, Anjana Mohandasan, J. Ephrem Nastasio, Maria Vittoria Legnardi
Poster for the Cool stars 20.5 virtual conference. Abstract: The amount of mass lost by stars during the red-giant branch (RGB) phase is one of the main parameters to correctly study later stages of stellar evolution. In spite of its importance, a fu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a5e2e0462105db74ff975d106e93046e
https://doi.org/10.5281/zenodo.4564645
https://doi.org/10.5281/zenodo.4564645
Autor:
E. P. Lagioia, Alvio Renzini, Sohee Jang, G. Cordoni, Anna F. Marino, Aaron Dotter, Amanda I. Karakas, M. Tailo, Marilia Carlos, Antonino Milone, E. Dondoglio
Multiple stellar populations (MPs) are a distinct characteristic of Globular Clusters (GCs). Their general properties have been widely studied among main sequence, red giant branch (RGB) and horizontal branch (HB) stars, but a common framework is sti
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::01f223674201ee307c3685c21e2720e5
http://arxiv.org/abs/2101.09843
http://arxiv.org/abs/2101.09843
Autor:
M. Tailo, Antonino Milone, G. Cordoni, E. P. Lagioia, Marilia Carlos, Anna F. Marino, E. Dondoglio, Sohee Jang
We exploit multi-band Hubble Space Telescope photometry to investigate multiple populations (MPs) along the red horizontal branches (HBs) and red clumps of fourteen metal-rich Globular Clusters (GCs), including twelve Milky Way GCs and the Magellanic
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e9ab716d3f0f9a857189b5a937a33953
http://arxiv.org/abs/2011.03283
http://arxiv.org/abs/2011.03283
Autor:
A. F. Marino, Alvio Renzini, E. P. Lagioia, Antonino Milone, M. Tailo, Marilia Carlos, E. Dondoglio, Chengyuan Li, S Jang, G. Cordoni
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Historically, photometry has been largely used to identify stellar populations (MPs) in Globular Clusters (GCs) by using diagrams that are based on colours and magnitudes that are mostly sensitive to stars with different metallicities or different ab
Autor:
Devika Kamath, D. A. García-Hernández, B. Cseh, Marilia Carlos, Maria Lugaro, Amanda I. Karakas
We present new theoretical stellar yields and surface abundances for asymptotic giant branch (AGB) models with a metallicity appropriate for stars in the Small Magellanic Cloud (SMC, $Z= 0.0028$, [Fe/H] $\approx -0.7$). New evolutionary sequences and
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1cbd16d0ce6ccdef0f53c26f694b8c85
Autor:
Fan Liu, Martin Asplund, David Yong, Amanda I. Karakas, Marilia Carlos, Anna F. Marino, Jorge Melendez, Ivan Ramirez
Publikováno v:
Repositório Institucional da USP (Biblioteca Digital da Produção Intelectual)
Universidade de São Paulo (USP)
instacron:USP
Universidade de São Paulo (USP)
instacron:USP
Stars in open clusters are expected to share an identical abundance pattern. Establishing the level of chemical homogeneity in a given open cluster deserves further study as it is the basis of the concept of chemical tagging to unravel the history of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6da736ca6c0b1d3ed9641211e16dc293
http://arxiv.org/abs/1608.03788
http://arxiv.org/abs/1608.03788