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20062009
most citedX-ray Variability in the Young Massive Triple theta2 Ori A

36 citations · 118 across the 6 of their papers we have counts for

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astro-ph20088 cited

Neon and Chemical Fractionation Trends in Late-type Stellar Atmospheres

D. Garcia-Alvarez, J. J. Drake, P. Testa

A survey of Ne, O and Fe coronal abundances culled from the recent literature for about 60 late-type stars confirms that the Ne/O ratio of stellar outer atmospheres is about two ti…

astro-ph200814 cited

Fe K alpha and hydrodynamic loop model diagnostics for a large flare on II Peg

Barbara Ercolano, Jeremy J. Drake, Fabio Reale +2

The observation by the Swift X-ray Telescope of the Fe K alpha_1, alpha_2 doublet during a large flare on the RS CVn binary system II Peg represents one of only two firm detections…

astro-ph200835 cited

Testing magnetically confined wind shock models for Beta Cep using XMM-Newton and Chandra phase-resolved X-ray observations

F. Favata, C. Neiner, P. Testa +2

(abridged) We have performed a set of phase-resolved X-ray observations of the magnetic B star Beta Cep, for which theoretical models predict the presence of a confined wind emitti…

astro-ph200825 cited

Geometry Diagnostics of a Stellar Flare from Fluorescent X-rays

P. Testa, J. J. Drake, B. Ercolano +5

We present evidence of Fe fluorescent emission in the Chandra HETGS spectrum of the single G-type giant HR 9024 during a large flare. In analogy to solar X-ray observations, we int…

astro-ph200725 cited

On X-ray Optical Depth in the Coronae of Active Stars

Paola Testa, Jeremy J. Drake, Giovanni Peres +1

We have investigated the optical thickness of the coronal plasma through the analysis of high-resolution X-ray spectra of a large sample of active stars observed with the High Ener…

astro-ph200636 cited

X-ray Variability in the Young Massive Triple theta2 Ori A

Norbert S. Schulz, Paola Testa, David P. Huenemoerder +2

Massive stars rarely show intrinsic X-ray variability. The only O-stars credited to be intrinsically variable are theta1 Ori C due to effects from magnetic confinement of its wind,…