104 citations · 295 across the 6 of their papers we have counts for
6 papers
Physicochemical models: source-tailored or generic?
Beatrice M. Kulterer, Maria N. Drozdovskaya, Audrey Coutens +2
Physicochemical models can be powerful tools to trace the chemical evolution of a protostellar system and allow to constrain its physical conditions at formation. The aim of this w…
The complex chemistry of hot cores in Sagittarius B2(N): Influence of cosmic-ray ionization and thermal history
M. Bonfand, A. Belloche, R. T. Garrod +4
As the number of complex organic molecules (COMs) detected in the interstellar medium increases, it becomes important to place meaningful constraints on the formation pathways of t…
Chemical modeling of internal photon-dominated regions surrounding deeply embedded HC/UCHII regions
Gwendoline Stéphan, Peter Schilke, Jacques Le Bourlot +4
We aim to investigate the chemistry of internal photon-dominated regions surrounding deeply embedded hypercompact and ultracompact HII regions. We search for specific tracers of th…
First detection of cyanamide (NHCN) towards solar-type protostars
A. Coutens, E. R. Willis, R. T. Garrod +11
Searches for the prebiotically-relevant cyanamide (NHCN) towards solar-type protostars have not been reported in the literature. We here present the first detection of this spe…
GHIGLS: HI mapping at intermediate Galactic latitude using the Green Bank Telescope
P. G. Martin, K. P. M. Blagrave, Felix J. Lockman +5
This paper introduces the data cubes from GHIGLS, deep Green Bank Telescope surveys of the 21-cm line emission of HI in 37 targeted fields at intermediate Galactic latitude. The GH…
Evolution of complex organic molecules in hot molecular cores: Synthetic spectra at (sub-)mm wavebands
Rumpa Choudhury, Peter Schilke, Gwendoline Stéphan +4
Hot molecular cores (HMCs) are intermediate stages of high-mass star formation and are also known for their rich emission line spectra at (sub-)mm wavebands. The observed spectral…