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20032009
most citedX-ray emission from classical T Tauri stars: Accretion shocks and coronae?

97 citations · 441 across the 11 of their papers we have counts for

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astro-ph200851 cited

Further X-ray detections of Herbig stars

B. Stelzer, J. Robrade, J. H. M. M. Schmitt +1

The interpretation of X-ray detections from Herbig Ae/Be stars is disputed as it is not clear if these intermediate-mass pre-main sequence stars are able to drive a dynamo and ensu…

astro-ph200811 cited

Quiescent X-ray emission from the M9 dwarf LHS 2065

J. Robrade, J. H. M. M. Schmitt

We investigate an archival XMM-Newton observation of LHS 2065, an ultracool dwarf with spectral type M9. We clearly detect LHS 2065 at soft X-ray energies in less than 1 h effectiv…

astro-ph200829 cited

Neon and oxygen in low activity stars: towards a coronal unification with the Sun

J. Robrade, J. H. M. M. Schmitt, F. Favata

The disagreement between helioseismology and a recent downward revision of solar abundances has resulted in a controversy about the true neon abundance of the Sun and other stars.…

astro-ph200722 cited

Doppler imaging an X-ray flare on the ultrafast rotator BO Mic - A contemporaneous multiwavelength study using XMM-Newton and VLT

U. Wolter, J. Robrade, J. H. M. M. Schmitt +1

We present an analysis of contemporaneous photospheric, chromospheric and coronal structures on the highly active K-dwarf star BO Mic (Speedy Mic). We localize a moderate flare in…

astro-ph200782 cited

X-rays from RU Lupi - Accretion and winds in CTTS

J. Robrade, J. H. M. M. Schmitt

Using three XMM-Newton observations we study the X-ray emission of RU Lup, a accreting and wind-driving CTTS. In comparison with other bright CTTS we study possible signatures of a…

astro-ph200797 cited

X-ray emission from classical T Tauri stars: Accretion shocks and coronae?

H. M. Guenther, J. H. M. M. Schmitt, J. Robrade +1

Classical T Tauri stars (CTTS) are surrounded by actively accreting disks. According to current models material falls along the magnetic field lines from the disk with more or less…