Searh results

Copertina volume box-s-2

HACK100

Volume 94, n. 2, 2023

Index
Foreword

Margherita’s work and legacys

P. SelvelliMargherita Hack: a life for science


DOI: https://doi.org/10.36116/MEMSAIT_94n2.2023.13
P. MolaroThe problem of Lithium and the other Light Elements Deuterium, Beryllium and Boron


DOI: https://doi.org/10.36116/MEMSAIT_94N2.2023.22
S. FerlugaThe strange Case of Epsilon Aurigae


DOI: https://doi.org/10.36116/MEMSAIT_94N2.2023.28
G. Umbriaco, A. Bianchini, A. Pizzella, A. et al.Margherita Hack’s Astrophysics at the Asiago Astrophysical Observatory


DOI: https://doi.org/10.36116/MEMSAIT_94N2.2023.34
M. MesserottiSolar radio observations in Trieste contributed to avert a nuclear war in 1967


DOI: https://doi.org/10.36116/MEMSAIT_94N2.2023.40
G. CatanzaroAm Stars: Abundances, ages, pulsations, and binarity


DOI: https://doi.org/10.36116/MEMSAIT_94N2.2023.50
P. Bonifacio, L. MonacoFeige 86: Gaia confirms its Horizontal Branch nature


DOI: https://doi.org/10.36116/MEMSAIT_94N2.2023.57
A. WolterA statue for Margherita


DOI: https://doi.org/10.36116/MEMSAIT_94N2.2023.61

Galactic archeology and formation of chemical elements

E. CaffauSearching for metal-poor stars


DOI: https://doi.org/10.36116/MEMSAIT_94N2.2023.68
J. I. González Hernández, D. S. Aguado, C. Allende-Prieto et al.Early phases of the Galaxy from the chemical imprint on the iron-poor stars J0815+4729 and J0023+0307


DOI: https://doi.org/10.36116/MEMSAIT_94N2.2023.77
I.Vanni, S. Salvadori, Á . SkúladóttirAre all metal-poor stars of second-generation?


DOI: https://doi.org/10.36116/MEMSAIT_94N2.2023.84
A. Bressan, G. Costa, S. Goswami, V. Grisoni, K. G. Shepherd, L. Silva, F. Addari, P. MarigoVery massive stars chemical enrichment in extremely metal-poor galaxies


DOI: https://doi.org/10.36116/MEMSAIT_94N2.2023.91
L. LombardoCERES survey: Stellar parameters and chemical abundances of selected elements


DOI: https://doi.org/10.36116/MEMSAIT_94N2.2023.99
F.-K. Thielemann, K. Farouqi, S. Rosswog, K.-L. KratzSources of r-Process Abundances


DOI: https://doi.org/10.36116/MEMSAIT_94N2.2023.105
M. Molero, D. Romano, M. Reichert,F. et al.Chemical evolution of Sagittarius: the heavy elements Eu and Ba


DOI: https://doi.org/10.36116/MEMSAIT_94N2.2023.118
A. Vasini, F. Matteucci, E. SpitoniChemical evolution of radioactive elements in the Milky Way


DOI: https://doi.org/10.36116/MEMSAIT_94N2.2023.123
F. MatteucciThe chemical evolution of the Milky Way: a problem of Galactic archaeology


DOI: https://doi.org/10.36116/MEMSAIT_94N2.2023.127
E. Spitoni, F. MatteucciThe [α/Fe] bimodality in the Milky Way disc with chemical evolution models


DOI: https://doi.org/10.36116/MEMSAIT_94N2.2023.134
S. Taibi, G. Battaglia, R. Leaman et al.Radial metallicity gradients of red giant stars in Local Group dwarf galaxies


DOI: https://doi.org/10.36116/MEMSAIT_94N2.2023.141
F. Z. MajidiCharacterization of YSOs with XSHOOTER


DOI: https://doi.org/10.36116/MEMSAIT_94N2.2023.147
A. HerreroA personal perspective on the history of massive OB stellar spectroscopy


DOI: https://doi.org/10.36116/MEMSAIT_94N2.2023.154
G. Costa, C. T. NguyenRotating stellar populations in NGC 1866: New PARSECv2.0 tracks with rotation


DOI: https://doi.org/10.36116/MEMSAIT_94N2.2023.167
A. Mucciarelli, D. MassariThe assembly history of the Local Group: the case of the Large Magellanic Cloud


DOI: https://doi.org/10.36116/MEMSAIT_94N2.2023.173

Exoplanets discovery and characterization

A. SozzettiPlanetary Systems Demographics: The View from High-Resolution Spectroscopy


DOI: https://doi.org/10.36116/MEMSAIT_94N2.2023.178
K. Biazzo & the GAPS TeamCharacterization of exoplanet hosting stars within the GAPS program


DOI: https://doi.org/10.36116/MEMSAIT_94N2.2023.189
S. Benatti, S. Desidera & the GAPS Young Objects TeamUnderstanding the evolution of planetary systems with GAPS2


DOI: https://doi.org/10.36116/MEMSAIT_94N2.2023.195
L. Silva, R. Bevilacqua, L. Biasiotti, E. et al.Climate and atmospheric models of rocky planets: habitability and observational properties


DOI: https://doi.org/10.36116/MEMSAIT_94N2.2023.203

Extragalactic Astronomy: Tracing the baryons- First Galaxies and their growth

C. PérouxThe Baryon Cycle


DOI: https://doi.org/10.36116/MEMSAIT_94N2.2023.211
S. Salvadori, V. D’Odorico, A. Saccardi, Á . Skúladóttir, I. VanniFirst stars signatures in high-z absorbers


DOI: https://doi.org/10.36116/MEMSAIT_94N2.2023.215
A. GrazianThe contribution of high-z AGN to the Ionizing UV background


DOI: https://doi.org/10.36116/MEMSAIT_94N2.2023.221
O. Cucciati, G. De Lucia, F. Fontanot, G. Zamorani, B.C. Lemaux, L. LubinGalaxy and structure formation before the cosmic noon. The perspective with galaxy spectroscopic surveys


DOI: https://doi.org/10.36116/MEMSAIT_94N2.2023.227
B.Vulcani, B. M. Poggianti, A. et al.Integral field spectroscopy allows us to distinguish among the different physical mechanisms affecting galaxies in the different environments


DOI: https://doi.org/10.36116/MEMSAIT_94N2.2023.233
R. Tripodi, C. Feruglio, F. Fiore, et al.ALMA unveils an outflow and a stellar bulge in an isolated z ∼ 6 QSO


DOI: https://doi.org/10.36116/MEMSAIT_94N2.2023.240
S. MaitraHigher order clustering of Lyα forest


DOI: https://doi.org/10.36116/MEMSAIT_94N2.2023.247

Cosmology and fundamental physics

S. Cristiani, K. Boutsia, G. Calderone, G. et al.Spectrographs and spectroscopists for the Sandage test


DOI: https://doi.org/10.36116/MEMSAIT_94N2.2023.251
M. Signorini, G. Risaliti, A. Sacchi, E. Lusso, E. NardiniBuilding the high-redshift Hubble Diagram with quasars


DOI: https://doi.org/10.36116/MEMSAIT_94N2.2023.259
P. Monaco on behalf of the Euclid ConsortiumMapping the Universe with slitless spectroscopy


DOI: https://doi.org/10.36116/MEMSAIT_94N2.2023.266
D. Milaković, C.C. Lee, P. Molaro, J.K. WebbMethods for quasar absorption system measurements of the fine structure constant in the 2020s and beyond


DOI: https://doi.org/10.36116/MEMSAIT_94N2.2023.270

Breakthrough science enabled by future spectrographs

S. Covino, S. Cristiani, J. M. Alcal´a, et al.CUBES: a UV spectrograph for the future


DOI: https://doi.org/10.36116/MEMSAIT_94N2.2023.281
C. NeinerUV spectropolarimetry: a new tool for breakthrough science


DOI: https://doi.org/10.36116/MEMSAIT_94N2.2023.294