activity
20012023
most citedAn Ice Age JWST inventory of dense molecular cloud ices

363 citations · 2.1k across the 47 of their papers we have counts for

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Showing 2020Show all

6 papers · 1 filter

astro-ph.SR2020★ 7 cited

On the Nature of the T Tauri Triple System

Tracy L. Beck, G. H. Schaefer, S. Guilloteau +4

We present a multi-wavelength analysis to reveal the nature of the enigmatic T Tauri triple star system. New optical and infrared measurements are coupled with archival X-ray, UV a…

astro-ph.SR2020

Possible Time Correlation Between Jet Ejection and Mass Accretion for RW Aur A

Michihiro Takami, Tracy L. Beck, P. Christian Schneider +17

For the active T-Taur star RW Aur A we have performed long-term (~10 yr) monitoring observations of (1) jet imaging in the [Fe II] 1.644-micron emission line using Gemini-NIFS and…

astro-ph.SR2020★ 16 cited

Orbital Motion, Variability, and Masses in the T Tauri Triple System

G. H. Schaefer, Tracy L. Beck, L. Prato +1

We present results from adaptive optics imaging of the T Tauri triple system obtained at the Keck and Gemini Observatories in 2015-2019. We fit the orbital motion of T Tau Sb relat…

astro-ph.SR2020★ 6 cited

Discovery of a jet from the single HAe/Be star HD 100546

P. C. Schneider, C. Dougados, E. T. Whelan +6

Young accreting stars drive outflows that collimate into jets, which can be seen hundreds of au from their driving sources. Accretion and outflow activity cease with system age, an…

astro-ph.EP2020★ 81 cited

Possible evidence of ongoing planet formation in AB Aurigae. A showcase of the SPHERE/ALMA synergy

A. Boccaletti, E. Di Folco, E. Pantin +8

Context. Planet formation is expected to take place in the first million years of a planetary system through various processes, which remain to be tested through observations. Aims…

astro-ph.SR2020★ 24 cited

GG Tau A: gas properties and dynamics from the cavity to the outer disk

N. T. Phuong, A. Dutrey, P. N. Diep +13

We used new ALMA CO and CO(3-2) observations obtained at high angular resolution (0.2") together with previous CO(3-2) and (6-5) ALMA data and continuum maps at…