Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
CAUP
SPACE, Univ. Nac. Mayor de San Marcos, Peru
Universidade do Porto, Portugal
Centro de Astrofisica da Universidade do Porto
IAG-USP
U. Nacional de San Marcos - Peru
Centro de Astrofisica, Universidade do Porto
Caltech / USA, Mt Stromlo / Australia
Centro de Astrofisica, Universidade de Porto, Portugal
Centro de Astrofísica da Universidade de Porto, Rua das Estrelas, 4150-762 Porto, Portugal
Instituto Astronomico e Geofisico, USP, Brazil
Centro de Astrofísica da Universidade do Porto, Rua das Estrelas, 4150-762 Porto, Portugal
Centro de Astrofisica da Universidade do Porto, Porto, Portugal
IAG / USP, 01060-970, São Paulo, Brazil
Departamento de Termodinámica y Fenómenos de Transferencia, Sartenejas, GFTUSB, Universidad Simón Bolívar
Caltech
Caltech, USA; UNMSM, Peru
RSAA, ANU
U.N.M. San Marcos, IMCA
IAG / Univ. Sao Paulo, now at Universidad Nacional Mayor de San Marcos, Lima, Peru
RSAA / ANU
IAG - Univ. Sao Paulo
RSAA, Australia
Centro de Astrofisica da Universidade de Porto
IAG / Universidade de Sao Paulo
Centro de Astrofísica da Universidade de Porto, Rua das Estrelas, 4150-762 Porto, Portugal de Sao Paulo
Research School of Astronomy and Astrophysics, The Australian National University, Cotter Road, Weston, ACT 2611, Australia
Universidad Nacional Mayor de San Marcos, Facultad de Ciencias Fisicas, Avenada Venezuela S / N, Ciudad Universitaria, Lima, Peru de Astrofísica, Universidade do Porto, Rua das Estrelas, 4150-762 Porto, Portugal de Astrofísica, Universidade do Porto, Rua das Estrelas, 4150-762 Porto, Portugal
Centro de Astrofísica da Universidade do Porto
A dedicated northern search for the first stars
A First Constraint on the Thick Disk Scale Length: Differential Radial Abundances in K Giants at Galactocentric Radii 4, 8, and 12 kpc
A High Primordial Lithium Abundance in Metal-Poor Stars
A library of high resolution synthetic stellar spectra from 300nm to 1.8 micron with solar and alpha-enhanced composition
A Low Solar Oxygen Abundance from the First Overtone OH Lines
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