activity
19992025
most citedEvidence for Accretion: High-Resolution X-ray Spectroscopy of the Classical T Tauri Star TW Hydrae

399 citations · 5.4k across the 153 of their papers we have counts for

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Showing 2013Show all

7 papers · 1 filter

astro-ph.SR2013★ 16 cited

Star Formation in Orion's L1630 Cloud: an Infrared and Multi-epoch X-ray Study

David A. Principe, Joel H. Kastner, Nicolas Grosso +4

X-ray emission is characteristic of young stellar objects (YSOs) and is known to be highly variable. We investigate, via an infrared and multi-epoch X-ray study of the L1630 dark c…

astro-ph.SR2013★ 1 cited

The magnetosphere of the close accreting PMS binary V4046 Sgr AB

S. G. Gregory, V. R. Holzwarth, J. -F. Donati +14

We present a preliminary 3D potential field extrapolation model of the joint magnetosphere of the close accreting PMS binary V4046 Sgr. The model is derived from magnetic maps obta…

astro-ph.SR2013★ 3 cited

The magnetosphere of the close accreting PMS binary V4046 Sgr

S. G. Gregory, V. R. Holzwarth, J. -F. Donati +14

V4046 Sagittarii AB is a close short-period classical T Tauri binary. It is a circularised and synchronised system accreting from a circumbinary disk. In 2009 it was observed as pa…

astro-ph.SR2013★ 103 cited

The Structure of the Evolved Circumbinary Disk around V4046 Sgr

Katherine A. Rosenfeld, Sean M. Andrews, David J. Wilner +2

We present sensitive, sub-arcsecond resolution Submillimeter Array observations of the protoplanetary disk around the nearby, pre-main sequence spectroscopic binary V4046 Sgr. We r…

astro-ph.SR2013★ 92 cited

The GALEX Nearby Young-Star Survey

David R. Rodriguez, B. Zuckerman, Joel H. Kastner +3

We describe a method that exploits data from the GALEX ultraviolet and WISE and 2MASS infrared source catalogs, combined with proper motions and empirical pre-main sequence isochro…

astro-ph.HE2013★ 15 cited

The Hot and Energetic Universe: Star formation and evolution

S. Sciortino, G. Rauw, M. Audard +16

Stars over a wide range of masses and evolutionary stages are nowadays known to emit X-rays. This X-ray emission is a unique probe of the most energetic phenomena occurring in the…