High angular resolution Australia Telescope Compact Array (ATCA) observations of SiO “thermal” millimetre line emission towards the two oxygen-rich, low mass loss rate AGB stars R Do
Context. The heavy mass loss observed in evolved asymptotic giant branch stars is usually attributed...
International audienceContext. The asymptotic giant branch (AGB) marks the final evolutionary stage ...
We present high angular resolution ( 0.2″) continuum and molecular emission line Atacama Large Milli...
Context. Asymptotic giant branch (AGB) stars go through a process of strong mass loss that involves ...
International audienceWe present the results of observations of the SiO masers at 7 mm wavelength in...
An extensive radiative transfer analysis of circumstellar SiO “thermal” radio line emission from a l...
© ESO 2018. Context. Low and intermediate mass stars are known to power strong stellar winds when e...
Aims. We present the results of observations with interferometers of a sample of pulsating asymptoti...
We present and analyse SO and SO2, recently observed with high angular resolution and sensitivity in...
We report the serendipitous detection with the Atacama Large Millimeter/submillimeter Array (ALMA) o...
Dedicated, unbiased spectral scans of asymptotic giant branch stars have so far been published only ...
The work presented in this thesis contributes to our understanding of the wind-driving mechanism and...
A conference in the honor of Hans Olofsson, Smögen, Sweden, August 27 - 29, 2019During the last deca...
Context. The heavy mass loss observed in evolved asymptotic giant branch stars is usually attributed...
Context. High angular resolution (sub)millimetre observations of asymptotic giant branch (AGB) stars...
Context. The heavy mass loss observed in evolved asymptotic giant branch stars is usually attributed...
International audienceContext. The asymptotic giant branch (AGB) marks the final evolutionary stage ...
We present high angular resolution ( 0.2″) continuum and molecular emission line Atacama Large Milli...
Context. Asymptotic giant branch (AGB) stars go through a process of strong mass loss that involves ...
International audienceWe present the results of observations of the SiO masers at 7 mm wavelength in...
An extensive radiative transfer analysis of circumstellar SiO “thermal” radio line emission from a l...
© ESO 2018. Context. Low and intermediate mass stars are known to power strong stellar winds when e...
Aims. We present the results of observations with interferometers of a sample of pulsating asymptoti...
We present and analyse SO and SO2, recently observed with high angular resolution and sensitivity in...
We report the serendipitous detection with the Atacama Large Millimeter/submillimeter Array (ALMA) o...
Dedicated, unbiased spectral scans of asymptotic giant branch stars have so far been published only ...
The work presented in this thesis contributes to our understanding of the wind-driving mechanism and...
A conference in the honor of Hans Olofsson, Smögen, Sweden, August 27 - 29, 2019During the last deca...
Context. The heavy mass loss observed in evolved asymptotic giant branch stars is usually attributed...
Context. High angular resolution (sub)millimetre observations of asymptotic giant branch (AGB) stars...
Context. The heavy mass loss observed in evolved asymptotic giant branch stars is usually attributed...
International audienceContext. The asymptotic giant branch (AGB) marks the final evolutionary stage ...
We present high angular resolution ( 0.2″) continuum and molecular emission line Atacama Large Milli...