activity
20082020
most citedWhere are the hot ion lines in classical T Tauri stars formed?

44 citations · 61 across the 2 of their papers we have counts for

collaborators

5 papers

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

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

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…

astro-ph.SR2018

A UV-to-NIR Study of Molecular Gas in the Dust Cavity Around RY Lupi

N. Arulanantham, K. France, K. Hoadley +10

We present a study of molecular gas in the inner disk around RY Lupi, with spectra from HST-COS, HST-STIS, and VLT-CRIRES. We model the radial d…

astro-ph200844 cited

Where are the hot ion lines in classical T Tauri stars formed?

H. M. Günther, J. H. M. M. Schmitt

Classical T Tauri stars show a plethora of in- and outflow signatures in a variety of wavelengths bands. In order to constrain gas velocities and temperatures we analyse the emissi…