Aims. We aim to investigate the physical and chemical properties of the molecular envelope of the oxygen-rich AGB star IK Ta
High angular resolution Australia Telescope Compact Array (ATCA) observations of SiO “thermal” milli...
During their late pulsating phase, AGB stars expel most of their mass in the form of massive dusty e...
Context. Unbiased spectral surveys are powerful tools to study the chemistry and the physics of star...
Aims. We aim to investigate the physical and chemical properties of the molecular envelope of the ox...
We carried out a millimeter wavelength line survey between 79 and 356 GHz with the IRAM-30m telescop...
[Aims] We aim to investigate the physical and chemical properties of the molecular envelope of the o...
Dedicated, unbiased spectral scans of asymptotic giant branch stars have so far been published only ...
Context. Molecular lines in the (sub)millimeter wavelength range can provide important information ...
International audienceDuring the late phases of low-intermediate mass (0.1 to 8 solar masses) stars,...
We have carried out a molecular line survey of the candidate massive protostar IRAS 23385+6053, cove...
A sensitive (1σ rms at 1 MHz resolution ~3 mK) 1 mm spectral line survey (214.5-285.5 GHz) of VY Can...
A conference in the honor of Hans Olofsson, Smögen, Sweden, August 27 - 29, 2019During the last deca...
Context. Unbiased spectral surveys are powerful tools to study the chemistry and the physics of star...
Context. The discovery of amino acids in meteorites fallen to Earth and the detection of glycine, th...
Context. The discovery of amino acids in meteorites fallen to Earth and the detection of glycine, th...
High angular resolution Australia Telescope Compact Array (ATCA) observations of SiO “thermal” milli...
During their late pulsating phase, AGB stars expel most of their mass in the form of massive dusty e...
Context. Unbiased spectral surveys are powerful tools to study the chemistry and the physics of star...
Aims. We aim to investigate the physical and chemical properties of the molecular envelope of the ox...
We carried out a millimeter wavelength line survey between 79 and 356 GHz with the IRAM-30m telescop...
[Aims] We aim to investigate the physical and chemical properties of the molecular envelope of the o...
Dedicated, unbiased spectral scans of asymptotic giant branch stars have so far been published only ...
Context. Molecular lines in the (sub)millimeter wavelength range can provide important information ...
International audienceDuring the late phases of low-intermediate mass (0.1 to 8 solar masses) stars,...
We have carried out a molecular line survey of the candidate massive protostar IRAS 23385+6053, cove...
A sensitive (1σ rms at 1 MHz resolution ~3 mK) 1 mm spectral line survey (214.5-285.5 GHz) of VY Can...
A conference in the honor of Hans Olofsson, Smögen, Sweden, August 27 - 29, 2019During the last deca...
Context. Unbiased spectral surveys are powerful tools to study the chemistry and the physics of star...
Context. The discovery of amino acids in meteorites fallen to Earth and the detection of glycine, th...
Context. The discovery of amino acids in meteorites fallen to Earth and the detection of glycine, th...
High angular resolution Australia Telescope Compact Array (ATCA) observations of SiO “thermal” milli...
During their late pulsating phase, AGB stars expel most of their mass in the form of massive dusty e...
Context. Unbiased spectral surveys are powerful tools to study the chemistry and the physics of star...