activity
20072010
most citedThe variable mass loss of the AGB star WX Psc as traced by the CO J=1-0 through 7-6 lines and the dust emission

43 citations · 169 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.SR2010★ 42 cited

Photometric multi-site campaign on the open cluster NGC 884 I. Detection of the variable stars

S. Saesen, F. Carrier, A. Pigulski +62

CONTEXT: Recent progress in the seismic interpretation of field beta Cep stars has resulted in improvements of the physics in the stellar structure and evolution models of massive…

astro-ph.SR2009★ 26 cited

Structure of the outer layers of cool standard stars

S. Dehaes, E. Bauwens, L. Decin +6

Context: Among late-type red giants, an interesting change occurs in the structure of the outer atmospheric layers as one moves to later spectral types in the Hertzsprung-Russell d…

astro-ph2008★ 33 cited

Detection of `parent' molecules from the inner wind of AGB stars as tracers of non-equilibrium chemistry

L. Decin, I. Cherchneff, S. Hony +3

Asymptotic Giant Branch (AGB) stars are typified by strong dust-driven, molecular outflows. For long, it was believed that the molecular setup of the circumstellar envelope of AGB…

astro-ph2007★ 43 cited

The variable mass loss of the AGB star WX Psc as traced by the CO J=1-0 through 7-6 lines and the dust emission

L. Decin, S. Hony, A. de Koter +3

Low and intermediate mass stars lose a significant fraction of their mass through a dust-driven wind during the Asymptotic Giant Branch (AGB) phase. Recent studies show that winds…

astro-ph2007★ 25 cited

Continuum emission around AGB stars at 1.2 mm

S. Dehaes, M. A. T. Groenewegen, L. Decin +3

It is generally acknowledged that the mass loss of Asymptotic Giant Branch (AGB) stars undergoes variations on different time scales. We constructed models for the dust envelopes f…