output
20022026
most citedGaia Data Release 2. Summary of the contents and survey properties

8.6k citations

Showing 2013Show all

105 papers · 1 filter

astro-ph.EP2013★ 30 cited

Origin of the peculiar eccentricity distribution of the inner cold Kuiper belt

A. Morbidelli, H. S. Gaspar, D. Nesvorny

Dawson and Murray-Clay (2012) pointed out that the inner part of the cold population in the Kuiper belt (that with semi major axis a<43.5 AU) has orbital eccentricities significant…

astro-ph.GA2013★ 47 cited

The Gaia-ESO Survey: Abundance ratios in the inner-disk open clusters Trumpler 20, NGC 4815, NGC 6705

L. Magrini, S. Randich, D. Romano +50

Open clusters are key tools to study the spatial distribution of abundances in the disk and their evolution with time. Using the first release of stellar parameters and abundances…

astro-ph.SR2013★ 100 cited

Measurement of acoustic glitches in solar-type stars from oscillation frequencies observed by Kepler

A. Mazumdar, M. J. P. F. G. Monteiro, J. Ballot +15

For the very best and brightest asteroseismic solar-type targets observed by Kepler, the frequency precision is sufficient to determine the acoustic depths of the surface convectiv…

astro-ph.SR2013★ 49 cited

The Gaia-ESO Survey: Reevaluation of the parameters of the open cluster Trumpler 20 using photometry and spectroscopy

P. Donati, T. Cantat-Gaudin, A. Bragaglia +34

Trumpler 20 is an old open cluster (OC) located toward the Galactic centre, at about 3 kpc from the Sun and 7 kpc from the Galactic centre. Its position makes this cluster pa…

astro-ph.SR2013★ 24 cited

A new procedure for defining a homogenous line-list for solar-type stars

S. G. Sousa, N. C. Santos, V. Adibekyan +9

Context. The homogenization of the stellar parameters is an important goal for large observational spectroscopic surveys, but it is very difficult to achieve it because of the dive…

astro-ph.SR2013★ 169 cited

Magnetic activity of F stars observed by Kepler

S. Mathur, R. A. Garcia, J. Ballot +6

The study of stellar activity is important because it can provide new constraints for dynamo models, when combined with surface rotation rates and the depth of the convection zone.…