activity
20062026
most citedChemistry of Dark Clouds: Databases, Networks, and Models

318 citations · 9.3k across the 181 of their papers we have counts for

collaborators
Showing 2012Show all

6 papers · 1 filter

astro-ph.EP2012★ 117 cited

The impact of atmospheric circulation on the chemistry of the hot Jupiter HD 209458b

M. Agundez, O. Venot, N. Iro +4

We investigate the effects of atmospheric circulation on the chemistry of the hot Jupiter HD 209458b. We use a simplified dynamical model and a robust chemical network, as opposed…

astro-ph.EP2012★ 255 cited

A chemical model for the atmosphere of hot Jupiters

Olivia Venot, Eric Hébrard, Marcelino Agùndez +5

Our purpose is to release a chemical network, and the associated rate coefficients, developed for the temperature and pressure range relevant to hot Jupiters atmospheres. Using thi…

astro-ph.GA2012★ 8 cited

Warm HCN in the planet formation zone of GV Tau N

Asunción Fuente, José Cernicharo, Marcelino Agúndez

The Plateau de Bure Interferometer has been used to map the continuum emission at 3.4 mm and 1.1 mm together with the J=1->0 and J=3->2 lines of HCN and HCO+ towards the binary sta…

astro-ph.GA2012★ 147 cited

Molecular abundances in the inner layers of IRC +10216

M. Agundez, J. P. Fonfria, J. Cernicharo +3

Observations towards IRC +10216 of CS, SiO, SiS, NaCl, KCl, AlCl, AlF, and NaCN have been carried out with the IRAM 30-m telescope in the 80-357.5 GHz frequency range. A large numb…

astro-ph.GA2012★ 21 cited

Herschel/HIFI observation of highly excited rotational lines of HNC toward IRC +10 216

F. Daniel, M. Agúndez, J. Cernicharo +6

We report the detection in emission of various highly excited rotational transitions of HNC (J = 6-5 through J =12-11) toward the carbon-star envelope IRC +10 216 using the HIFI in…

astro-ph.SR2012★ 42 cited

On the physical structure of IRC+10216. Ground-based and Herschel observations of CO and CCH

E. De Beck, R. Lombaert, M. Agúndez +17

The C-rich AGB star IRC+10216 undergoes strong mass loss, and quasi-periodic density enhancements in the circumstellar matter have been reported. CO is ubiquitous in the CSE, while…