Stellar population astrophysics (SPA) with the TNG: Revisiting the metallicity of Praesepe (M 44)

被引：0

作者：

D'Orazi, V. ^{[1
,2
]}

Oliva, E. ^{[3
]}

Bragaglia, A. ^{[4
]}

Frasca, A. ^{[5
]}

Sanna, N. ^{[3
]}

Biazzo, K. ^{[5
]}

Casali, G. ^{[3
]}

Desidera, S. ^{[1
]}

Lucatello, S. ^{[1
]}

Magrini, L. ^{[3
]}

Origlia, L. ^{[4
]}

机构：

[1] INAF Osservatorio Astronomico di Padova, Vicolo dell'Osservatorio 5, Padova,35122, Italy

[2] Monash Centre for Astrophysics, School of Physics and Astronomy, Monash University, Melbourne,VIC,3800, Australia

[3] INAF Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, Firenze,50125, Italy

[4] INAF Osservatorio di Astrofisica e Scienza Dello Spazio di Bologna, Via Gobetti 93/3, Bologna,40129, Italy

[5] INAF Osservatorio Astrofisico di Catania, Via S. Sofia 78, Catania,95123, Italy

来源：

Astronomy and Astrophysics | 2020年 / 633卷

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摘要：

Journal article (JA)

引用

共 16 条

[1] Stellar population astrophysics (SPA) with the TNG Revisiting the metallicity of Praesepe (M 44)
D'Orazi, V.
Oliva, E.
Bragaglia, A.
Frasca, A.
Sanna, N.
Biazzo, K.
Casali, G.
Desidera, S.
Lucatello, S.
Magrini, L.
Origlia, L.
ASTRONOMY & ASTROPHYSICS, 2020, 633
[2] Stellar Population Astrophysics (SPA) with TNG
Seshashayana, S. Bijavara
Jonsson, H.
D'Orazi, V.
Nandakumar, G.
Oliva, E.
Bragaglia, A.
Sanna, N.
Romano, D.
Spitoni, E.
Karakas, A.
Lugaro, M.
Origlia, L.
ASTRONOMY & ASTROPHYSICS, 2024, 683
[3] Stellar population astrophysics (SPA) with the TNG The Arcturus Lab
Fanelli, C.
Origlia, L.
Oliva, E.
Mucciarelli, A.
Sanna, N.
Dalessandro, E.
Romano, D.
ASTRONOMY & ASTROPHYSICS, 2021, 645
[4] Stellar population astrophysics with the TNG
Vernekar, Nagaraj
Lucatello, Sara
Bragaglia, Angela
Miglio, Andrea
Sanna, Nicoletta
Andreuzzi, Gloria
Frasca, Antonio
ASTRONOMY & ASTROPHYSICS, 2024, 684
[5] Stellar population astrophysics (SPA) with the TNG The chemical content of the red supergiant population in the Perseus
Fanelli, C.
Origlia, L.
Oliva, E.
Dalessandro, E.
Mucciarelli, A.
Sanna, N.
ASTRONOMY & ASTROPHYSICS, 2022, 660
[6] Stellar population astrophysics (SPA) with the TNG Characterization of the young open cluster ASCC 123
Frasca, A.
Alonso-Santiago, J.
Catanzaro, G.
Bragaglia, A.
Carretta, E.
Casali, G.
D'Orazi, V
Magrini, L.
Andreuzzi, G.
Oliva, E.
Origlia, L.
Sordo, R.
Vallenari, A.
ASTRONOMY & ASTROPHYSICS, 2019, 632
[7] Stellar Population Astrophysics (SPA) with TNG Atmospheric parameters of members of 16 unstudied open clusters
Zhang, R.
Lucatello, S.
Bragaglia, A.
Carrera, R.
Spina, L.
Alonso-Santiago, J.
Andreuzzi, G.
Casali, G.
Carretta, E.
Frasca, A.
Fu, X.
Magrini, L.
Origlia, L.
D'Orazi, V
Vallenari, A.
ASTRONOMY & ASTROPHYSICS, 2021, 654
[8] Stellar Population Astrophysics (SPA) with the TNG a-elements, lithium, sodium and aluminum in 16 open clusters
Zhang, R.
Lucatello, S.
Bragaglia, A.
Alonso-Santiago, J.
Andreuzzi, G.
Casali, G.
Carrera, R.
Carretta, E.
D'Orazi, V.
Frasca, A.
Fu, X.
Magrini, L.
Minchev, I
Origlia, L.
Spina, L.
Vallenari, A.
ASTRONOMY & ASTROPHYSICS, 2022, 667
[9] Stellar Population Astrophysics (SPA) with the TNG Stock 2, a little-studied open cluster with an eMSTO
Alonso-Santiago, J.
Frasca, A.
Catanzaro, G.
Bragaglia, A.
Andreuzzi, G.
Carrera, R.
Carretta, E.
Casali, G.
D'Orazi, V
Fu, X.
Giarrusso, M.
Lucatello, S.
Magrini, L.
Origlia, L.
Spina, L.
Vallenari, A.
Zhang, R.
ASTRONOMY & ASTROPHYSICS, 2021, 656
[10] Stellar population astrophysics (SPA) with the TNG Identification of a sulphur line at λair=1063.6 nm in GIANO-B stellar spectra
Ryde, N.
Hartman, H.
Oliva, E.
Origlia, L.
Sanna, N.
Rainer, M.
Thorsbro, B.
Dalessandro, E.
Bono, G.
ASTRONOMY & ASTROPHYSICS, 2019, 631

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