activity
20042009
most citedEvidence for Accretion in the High-resolution X-ray Spectrum of the T Tauri Star System Hen 3-600

68 citations · 274 across the 10 of their papers we have counts for

collaborators

14 papers

astro-ph.HE2009

Structure and Evolution of Pre-Main Sequence Stars

Norbert S. Schulz, Glenn Allen, Mark W. Bautz +28

Low-mass pre-main sequence (PMS) stars are strong and variable X-ray emitters, as has been well established by EINSTEIN and ROSAT observatories. It was originally believed that thi…

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-ph200819 cited

X-ray Emission from Young Stellar Objects in the εChamaeleontis Group: the Herbig Ae Star HD 104237 and Associated Low-Mass Stars

Paola Testa, David P. Huenemoerder, Norbert S. Schulz +1

We present Chandra-HETGS observations of the Herbig Ae star HD 104237 and the associated young stars comprising lower mass stars, in the 0.15-1.75\msol mass range, in their pre-mai…

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-ph200768 cited

Evidence for Accretion in the High-resolution X-ray Spectrum of the T Tauri Star System Hen 3-600

David P. Huenemoerder, Joel H. Kastner, Paola Testa +2

We present high-resolution X-ray spectra of the multiple T Tauri star system Hen 3-600, obtained with the High Energy Transmission Grating Spectrograph on the Chandra X-ray Observa…

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…