activity
20042025
most citedA New Probe of the Planet-Forming Region in T Tauri Disks

117 citations · 820 across the 15 of their papers we have counts for

collaborators

15 papers

astro-ph.GA2025★ 3 cited

A Tentative Detection of Molecular Hydrogen (H) Emission Lines at Cosmic Dawn

Madisen Johnson, Blakesley Burkhart, Francesco D'Eugenio +11

We present a theoretical framework for interpreting far-ultraviolet (FUV) fluorescent emission from molecular hydrogen (H) in high-redshift galaxies, motivated by the unique ca…

astro-ph.GA2023★ 1 cited

Analysis of the first infrared spectrum of quasi-bound H2 line emission in Herbig-Haro 7

Evelyne Roueff, Michael G. Burton, Thomas R. Geballe +1

Context. Highly excited molecular hydrogen H2 has been observed in many regions of shocked molecular gas. A recently published -band spectrum of Herbig-Haro 7 (HH7) contains sev…

astro-ph.GA2022★ 1 cited

The quasi bound spectrum of H2

E. M. Roueff, H. Abgrall

We compute the radiative ro-vibrational emission spectrum of H2 involving quasibound states via a simple numerical method of resolution of the Schrödinger equation by introducing a…

physics.atom-ph2019★ 110 cited

The full infrared spectrum of molecular hydrogen

E. Roueff, H. Abgrall, P. Czachorowski +3

The high spectral resolution R about 45,000 provided by IGRINS (Immersion Grating INfrared Spectrometer) at MacDonald Observatory and R 100,000 achieved by CRIRES (CRyogenic high-r…

astro-ph.CO2018★ 12 cited

H/HD molecular data for analysis of quasar spectra in search of varying constants

W. Ubachs, E. J. Salumbides, M. T. Murphy +2

Absorption lines of H and HD molecules observed at high redshift in the line of sight towards quasars are a test ground to search for variation of the proton-to-electron mass r…

astro-ph.SR2017★ 28 cited

The 1600 Angstrom Emission Bump in Protoplanetary Disks: A Spectral Signature of HO Dissociation

Kevin France, Evelyne Roueff, Herve Abgrall

The FUV continuum spectrum of many accreting pre-main sequence stars, Classical T Tauri Stars (CTTSs), does not continue smoothly from the well-studied Balmer continuum emission in…