activity
20002009
most citedEvidence for Accretion in the High-resolution X-ray Spectrum of the T Tauri Star System Hen 3-600

68 citations · 115 across the 4 of their papers we have counts for

collaborators

9 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-ph20083 cited

Spatially-resolved Chandra Imaging Spectroscopy of the classical/weak-lined T Tauri system V710 Tau

Sonali J. Shukla, David A. Weintraub, Joel H. Kastner

We present spatially-resolved X-ray observations of the binary T Tauri star system V710 Tau. Using Chandra's Advanced CCD Imaging Spectrometer (ACIS), we imaged this 3.2'' separati…

astro-ph200844 cited

Quiescent H2 Emission From Pre-Main Sequence Stars in Chamaeleon I

Jeffrey S. Bary, David A. Weintraub, Sonali J. Shukla +2

We report the discovery of quiescent emission from molecular hydrogen gas located in the circumstellar disks of six pre-main sequence stars, including two weak-line T Tauri stars (…

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-ph2005

Enhanced X-ray variability from V1647 Ori, the young star in outburst illuminating McNeil's Nebula

N. Grosso, J. H. Kastner, H. Ozawa +5

We report a ~38 ks X-ray observation of McNeil's Nebula obtained with XMM on 2004 April 4. V1647 Ori, the young star in outburst illuminating McNeil's Nebula, is detected with XMM…

astro-ph2004

An X-ray Outburst from the Rapidly Accreting Young Star That Illuminates McNeil's Nebula

J. H. Kastner, M. Richmond, N. Grosso +6

Young, low-mass stars are luminous X-ray sources whose powerful X-ray flares may exert a profound influence over the process of planet formation. The origin of such emission is unc…