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20002026
most citedThe Origin of T Tauri X-ray Emission: New Insights from the Chandra Orion Ultradeep Project

534 citations · 8.5k across the 132 of their papers we have counts for

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Showing 2010Show all

6 papers · 1 filter

astro-ph.SR2010

Young Stars in the Time Domain: A Cool Stars 16 Splinter Summary

Kevin R. Covey, Peter Plavchan, Fabienne Bastien +6

Variability is a defining characteristic of young stellar systems, and optical variability has been heavily studied to select and characterize the photospheric properties of young…

astro-ph.SR2010★ 1 cited

Time-resolved spectroscopy of DROXO X-ray sources: Flares and FeKalpha emission

B. Stelzer, E. Flaccomio, I. Pillitteri +2

We present a systematic search for Fe Kalpha emission from young stellar objects of the rho Ophiuchi star forming region observed in the Deep Rho Ophiuchi XMM-Newton Observation (D…

astro-ph.SR2010★ 124 cited

Non-stationary dynamo & magnetospheric accretion processes of the classical T Tauri star V2129 Oph

JF Donati, J Bouvier, FM Walter +11

We report here the first results of a multi-wavelength campaign focussing on magnetospheric accretion processes of the classical TTauri star (cTTS) V2129Oph. In this paper, we pres…

astro-ph.SR2010★ 19 cited

Correlated optical and X-ray variability in CTTS - Indications of absorption-modulated emission

E. Flaccomio, G. Micela, F. Favata +1

Optical and X-ray emission from classical T Tauri stars (CTTSs) has long been known to be highly variable. Our long, uninterrupted optical observation of the NGC2264 region with Co…

astro-ph.SR2010★ 159 cited

Accretion dynamics and disk evolution in NGC 2264: a study based on the Corot photometric observations

S. H. P. Alencar, P. S. Teixeira, M. M. Guimaraes +6

The young cluster NGC 2264 was observed with the Corot satellite for 23 days uninterruptedly in March 2008 with unprecedent photometric accuracy. We present here the first results…

astro-ph.SR2010★ 29 cited

Results from DROXO. III. Observation, source list and X-ray properties of sources detected in the "Deep Rho Ophiuchi XMM-Newton Observation"

I. Pillitteri, S. Sciortino, E. Flaccomio +8

X-rays from very young stars are powerful probes to investigate the mechanisms at work in the very first stages of the star formation and the origin of X-ray emission in very young…