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

collaborators

154 papers

astro-ph.EP2025

The Age and High Energy Environment of the Very Young Transiting Exoplanet TOI 1227b

Attila Varga, Joel H. Kastner, Alexander S. Binks +2

The mid-M star TOI~1227 hosts among the youngest known transiting exoplanets. We have conducted new X-ray imaging and optical spectroscopic observations of TOI 1227 aimed at ascert…

astro-ph.SR2024★ 3 cited

Walking the Line: Young Stars on the Boundary of the Epsilon Cha and Lower Centaurus-Crux Associations

Attila Varga, Joel H. Kastner, D. Annie Dickson-Vandervelde +1

Gaia Data Release 3 (DR3) has provided the largest and most astrometrically precise catalogue of nearby stars to date, allowing for a more complete membership census of nearby, you…

astro-ph.SR2024

Asymptotic giant branch stars in the eROSITA-DE eRASS1 catalog

Martin A. Guerrero, Rodolfo Montez, Roberto Ortiz +2

AGB stars are not expected to be X-ray-emitters, yet a small fraction of them, the so-called X-AGBs, show X-ray emission that can be attributed to coronal activity of a companion o…

astro-ph.SR2024

The Molecular Exoskeleton of the Ring-like Planetary Nebula NGC 3132

Joel H. Kastner, David Wilner, Paula Moraga Baez +4

We present Submillimeter Array (SMA) mapping of CO , CO , and CN emission from the Ring-like planetary nebula (…

astro-ph.SR2023★ 1 cited

Twenty-Five Years of Accretion onto the Classical T Tauri Star TW Hya

Gregory J. Herczeg, Yuguang Chen, Jean-Francois Donati +39

Accretion plays a central role in the physics that governs the evolution and dispersal of protoplanetary disks. The primary goal of this paper is to analyze the stability over time…

astro-ph.EP2023★ 17 cited

Spirals and clumps in V960 Mon: signs of planet formation via gravitational instability around an FU Ori star?

P. Weber, S. Pérez, A. Zurlo +11

The formation of giant planets has traditionally been divided into two pathways: core accretion and gravitational instability. However, in recent years, gravitational instability h…