activity
20162024
most citedImaging the water-snow line during a protostellar outburst

234 citations · 312 across the 9 of their papers we have counts for

collaborators

10 papers

astro-ph.IM2024

Sherpa: An Open Source Python Fitting Package

Aneta Siemiginowska, Douglas Burke, Hans Moritz Günther +8

We present an overview of Sherpa, an open source Python project, and discuss its development history, broad design concepts and capabilities. Sherpa contains powerful tools for com…

astro-ph.SR2024

The environment around young eruptive stars. SPHERE/IRDIS polarimetric imaging of 7 protostars

A. Zurlo, P. Weber, S. Pérez +11

Eruptive stars are a class of young stellar objects that show an abrupt increase in their luminosity. These burst-like episodes are thought to dominate the stellar accretion proces…

astro-ph.IM20231 cited

The life cycle of stars and their planets from the high energy perspective

Lia Corrales, Keivan G. Stassun, Tim Cunningham +19

One of the key research themes identified by the Astro2020 decadal survey is Worlds and Suns in Context. The Advanced X-ray Imaging Satellite (AXIS) is a proposed NASA APEX mission…

astro-ph.SR20231 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.SR2023

Stable Coronal X-Ray Emission Over Twenty Years of XZ Tau

Steven M. Silverberg, Hans Moritz Guenther, Pragati Pradhan +3

XZ Tau AB is a frequently observed binary YSO in the Taurus Molecular Cloud; XZ Tau B has been classified as an EXOr object. We present new Chandra/HETG-ACIS-S observations of XZ T…

astro-ph.EP202317 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…