most citedThe UV Perspective of Low-Mass Star Formation

17 citations · 23 across the 2 of their papers we have counts for

collaborators

7 papers

astro-ph.SR20206 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.SR202017 cited

The UV Perspective of Low-Mass Star Formation

P. C. Schneider, H. M. Günther, K. France

The formation of low-mass stars in molecular clouds involves accretion disks and jets, which are of broad astrophysical interest. Accreting stars represent the closest examples of…

astro-ph.SR2020

Spatially resolved velocity structure in jets of DF Tau and UY Aur A

Anastasiia V Uvarova, Hans Moritz Günther, David A. Principe +1

Young stars accrete mass and angular momentum from their circumstellar disks. Some of them also drive outflows, which can be distinguished in optical forbidden emission lines (FELs…

astro-ph.SR2020

Probing UV-Sensitive Pathways for CN and HCN Formation in Protoplanetary Disks with the Hubble Space Telescope

Nicole Arulanantham, K. France, P. Cazzoletti +6

The UV radiation field is a critical regulator of gas-phase chemistry in surface layers of disks around young stars. In an effort to understand the relationship between photocataly…

astro-ph.SR2018

Optical dimming of RW Aur associated with an iron rich corona and exceptionally high absorbing column density

Hans Moritz Günther, T. Birnstiel, D. P. Huenemoerder +7

RW Aur is a binary system composed of two young, low-mass stars. The primary, RW Aur A, has undergone visual dimming events (~mag) in 2011, 2014-16, and 2017-2018. Visual…

astro-ph.SR2018

Multiepoch, multiwavelength study of accretion onto T Tauri: X-ray versus optical and UV accretion tracers

P. C. Schneider, H. M. Günther, J. Robrade +2

Classical T Tauri stars (CTTSs) accrete matter from the inner edge of their surrounding circumstellar disks. The impact of the accretion material on the stellar atmosphere results…