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20012022
most citedA correlation between the heavy element content of transiting extrasolar planets and the metallicity of their parent stars

332 citations · 3.8k across the 70 of their papers we have counts for

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Showing astro-ph.SRShow all

15 papers · 1 filter

astro-ph.SR2021★ 39 cited

Evidence for an MHD disk wind via optical forbidden line spectro-astrometry

E. T Whelan, I. Pascucci, U. Gorti +4

Spectro-astrometry is used to investigate the low velocity component (LVC) of the optical forbidden emission from the T Tauri stars RU Lupi and AS 205 N. Both stars also have high…

astro-ph.SR2020★ 47 cited

Search for associations containing young stars (SACY) VIII. An updated census of spectroscopic binary systems showing hints of non-universal multiplicity among these associations

S. Zúñiga-Fernández, A. Bayo, P. Elliott +10

We seek to update the spectroscopy binary fraction of the SACY (Search for Associations Containing Young stars) sample taking in consideration all possible biases in our identifica…

astro-ph.SR2018★ 4 cited

On the incidence of planet candidates in open clusters and a planet confirmation

I. C. Leão, B. L. Canto Martins, S. Alves +7

Detecting exoplanets in clusters of different ages is a powerful tool for understanding a number of open questions, such as how the occurrence rate of planets depends on stellar me…

astro-ph.SR2016★ 3 cited

Fundamental stellar parameters for selected T-Tauri stars in the Chamaeleon and Rho Ophiuchus star-forming regions

David James, Alicia Aarnio, Alexander Richert +4

We present the results of an optical photometry and high-resolution spectroscopy campaign for a modest sample of X-ray selected stars in the Chamaeleon and Rho Ophiuchus star formi…

astro-ph.SR2015★ 11 cited

Physical parameters and long-term photometric variability of V1481 Ori, a SB2 member of Orion Nebula Cluster with an accreting component

Sergio Messina, Padmakar Parihar, Katia Biazzo +5

We present the results of our analysis on V1481 Ori (JW 239), a young SB2 in the Orion Nebula Cluster with a circumbinary disc accreting on the lower-mass component. The analysis i…

astro-ph.SR2015★ 6 cited

WISE J061213.85-303612.5: a new T-dwarf binary candidate

N. Huélamo, V. D. Ivanov, R. Kurtev +8

T and Y-dwarfs are among the coolest and least luminous objects detected, and they can help to understand the properties of giant planets. Their multiplicity properties can shed li…