activity
20152021
most citedDiscovery of a warm, dusty giant planet around HIP65426

205 citations · 937 across the 21 of their papers we have counts for

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Showing astro-ph.SRShow all

7 papers · 1 filter

astro-ph.SR20209 cited

Investigating three Sirius-like systems with SPHERE

R. Gratton, V. D'Orazi, T. A. Pacheco +61

Sirius-like systems are wide binaries composed of a white dwarf (WD) and a companion of a spectral type earlier than M0. The WD progenitor evolves in isolation, but its wind during…

astro-ph.SR20195 cited

Investigating the nature of the extended structure around the Herbig star RCrA using integral field and high-resolution spectroscopy

E. Rigliaco, R. Gratton, D. Mesa +24

We present a detailed analysis of the extended structure detected around the young and close-by Herbig Ae/Be star RCrA. This is a young triple system with an intermediate mass cent…

astro-ph.SR2019

The origin of R CrA variability: A complex triple system hosting a disk

E. Sissa, R. Gratton, J. M. Alcala +5

R~CrA is the brightest member of the Coronet star forming region and it is the closest Herbig AeBe star with a spectrum dominated by emission lines. Its luminosity has been monitor…

astro-ph.SR201928 cited

Exploring the RCrA environment with SPHERE: Discovery of a new stellar companion

D. Mesa, M. Bonnefoy, R. Gratton +39

Aims. R Coronae Australis (R CrA) is the brightest star of the Coronet nebula of the Corona Australis (CrA) star forming region. It has very red colors, probably due to dust absorp…

astro-ph.SR201849 cited

SPHERE dynamical and spectroscopic characterization of HD142527B

R. Claudi, A. -L. Maire, D. Mesa +50

We detect the accreting low-mass companion HD142527B at a separation of 73 mas (11.4 au) from the star. No other companions with mass greater than 10 MJ are visible in the field of…

astro-ph.SR2018

Mapping of shadows cast on a protoplanetary disk by a close binary system

V. D'Orazi, R. Gratton, S. Desidera +47

For a comprehensive understanding of planetary formation and evolution, we need to investigate the environment in which planets form: circumstellar disks. Here we present high-cont…