activity
20102016
most citedConstraints on the H2O formation mechanism in the wind of carbon-rich AGB stars

21 citations · 21 across the 1 of their papers we have counts for

collaborators

9 papers

astro-ph.SR2016★ 21 cited

Constraints on the H2O formation mechanism in the wind of carbon-rich AGB stars

R. Lombaert, L. Decin, P. Royer +13

Context. The recent detection of warm HO vapor emission from the outflows of carbon-rich asymptotic giant branch (AGB) stars challenges the current understanding of circumstell…

astro-ph.SR2013

HIFISTARS Herschel/HIFI observations of VY Canis Majoris. Molecular-line inventory of the envelope around the largest known star

J. Alcolea, V. Bujarrabal, P. Planesas +16

To gain insight into the physical conditions and kinematics of the warm (100-1000 K) gas around the red hyper-giant VY CMa, we performed sensitive high spectral resolution observat…

astro-ph.SR2011

Herschel/HIFI observations of O-rich AGB stars : molecular inventory

K. Justtanont, T. Khouri, M. Maercker +15

Spectra, taken with the heterodyne instrument, HIFI, aboard the Herschel Space Observatory, of O-rich asymptotic giant branch (AGB) stars which form part of the guaranteed time key…

astro-ph.SR2011

Herschel/HIFI observations of molecular emission in protoplanetary nebulae and young planetary nebulae

V. Bujarrabal, J. Alcolea, R. Soria-Ruiz +1

We performed Herschel/HIFI observations of intermediate-excitation molecular lines in the far-infrared/submillimeter range in a sample of ten protoplanetary nebulae and young plane…

astro-ph.SR2010

Herschel/HIFI deepens the circumstellar NH3 enigma

K. M. Menten, F. Wyrowski, J. Alcolea +23

Circumstellar envelopes (CSEs) of a variety of evolved stars have been found to contain ammonia (NH3) in amounts that exceed predictions from conventional chemical models by many o…

astro-ph.SR2010

Herschel/HIFI observations of high-J CO transitions in the protoplanetary nebula CRL618

V. Bujarrabal, J. Alcolea, R. Soria-Ruiz +25

We performed Herschel/HIFI observations of several CO lines in the far-infrared/sub-mm in the protoplanetary nebula CRL618. The high spectral resolution provided by HIFI allows mea…