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20012023
most citedGaia Data Release 2. Summary of the contents and survey properties

8.6k citations · 15.7k across the 64 of their papers we have counts for

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17 papers · 1 filter

astro-ph2008★ 21 cited

Blue Straggler Stars in Galactic Open Clusters and the effect of field star contamination

G. Carraro, R. A. Vazquez, A. Moitinho

We investigate the distribution of Blue Straggler stars in the field of three open star clusters. The main purpose is to highlight the crucial role played by general Galactic disk…

astro-ph2008

Milli-arcsecond astrophysics with VSI, the VLTI spectro-imager in the ELT era

F. Malbet, D. Buscher, G. Weigelt +49

Nowadays, compact sources like surfaces of nearby stars, circumstellar environments of stars from early stages to the most evolved ones and surroundings of active galactic nuclei c…

astro-ph2008★ 17 cited

Stellar populations in the Canis Major over-density

Giovanni Carraro, Andre' Moitinho, Ruben A. Vazquez

We performed a photometric multicolor survey of the core of the Canis Major over-density at l 244, -8.0, reaching V = 22 and covering 0.3 x 1 degree. The main aim is to unravel the…

astro-ph2007★ 103 cited

Spiral structure in the outer Galactic disk. I. The Third Galactic Quadrant

Ruben A. Vazquez, Jorge May, Giovanni Carraro +3

We combine optical and radio observations to trace the spiral structure in the Third Quadrant of the Milky Way. The optical observations consist of a large sample of young open clu…

astro-ph2006★ 18 cited

Photometry of a Galactic field at l = 232, b = -6. The old open cluster Auner 1, the Norma-Cygnus spiral arm and the signature of the warped Galactic Thick Disk

Giovanni Carraro, Andre' Moitinho, Manuela Zoccali +2

We perform a detailed photometric study of the stellar populations in a Galactic Field at l = 232, b = -6 in the Canis Major (CMa) constellation. We present the first U,B,V,I photo…

astro-ph2006★ 62 cited

On the difference between nuclear and contraction ages

W. Lyra, A. Moitinho, N. van der Bliek +1

Context:Ages derived from the low mass stars still contracting onto the main sequence often differ from ages derived from the high mass ones that have already evolved away from it.…