output
19962026
most citedGaia Data Release 2. Summary of the contents and survey properties

8.6k citations

Showing 2020 · astro-ph.SRShow all

22 papers · 2 filters

astro-ph.SR2020★ 340 cited

Gaia Early Data Release 3: The Gaia Catalogue of Nearby Stars

Gaia Collaboration, R. L. Smart, L. M. Sarro +420

We produce a clean and well-characterised catalogue of objects within 100\,pc of the Sun from the \G\ Early Data Release 3. We characterise the catalogue through comparisons to the…

astro-ph.SR2020★ 3 cited

Velocity-intensity asymmetry reversal of solar radial p-modes

J. Philidet, K. Belkacem, H. -G. Ludwig +2

The development of space-borne missions has significantly improved the quality of the measured spectra of solar-like oscillators. Their -mode line profiles can now be resolved,…

astro-ph.SR2020★ 10 cited

The nearby magnetic cool DZ white dwarf PM J08186-3110

Adela Kawka, Stéphane Vennes, Nicole F. Allard +2

We present an analysis of photometric, spectroscopic and spectropolarimetric data of the nearby, cool, magnetic DZ white dwarf PM J08186-3110. High dispersion spectra show the pres…

astro-ph.SR2020★ 37 cited

The solar gravitational redshift from HARPS-LFC Moon spectra. A test of the General Theory of Relativity

J. I. González Hernández, R. Rebolo, L. Pasquini +15

The General Theory of Relativity predicts the redshift of spectral lines in the solar photosphere, as a consequence of the gravitational potential of the Sun. This effect can be me…

astro-ph.SR2020★ 25 cited

Mono-enriched stars and Galactic chemical evolution -- Possible biases in observations and theory

Camilla Juul Hansen, Andreas Koch, Lyudmila Mashonkina +9

A long sought after goal using chemical abundance patterns derived from metal-poor stars is to understand the Galactic chemical evolution (GCE) and to pin down the nature of the fi…

astro-ph.SR2020★ 2 cited

The GRAVITY young stellar object survey III. The dusty disk of RY Lup

GRAVITY Collaboration, Y. -I. Bouarour, K. Perraut +55

We use PIONIER data from the ESO archive and GRAVITY data that were obtained in June 2017 with the four 8m telescopes. We use a parametric disk model and the 3D radiative transfer…