Add to ORKGWe present new Herschel HIFI (de Graauw et al. 2010) and PACS (Poglitsch et al. 2010) sub-millimeter and far-infrared line observations of several molecular species towards the S-type AGB star W Aql. We use these observations, which probe a wide range of gas temperatures, to constrain the circumstellar properties of W Aql, including mass-loss rate and molecular abundances.status: publishe
Aims. A set of new, sensitive, and spectrally resolved, sub-millimeter line observations are used to...
Aims. A set of new, sensitive, and spectrally resolved, sub-millimeter line observations are used to...
Detailed modelling of the circumstellar molecular line emission of the S-type AGB star W Aquilae
We present new Herschel(1) HIFI (de Graauw et al. 2010) and PACS (Poglitsch et al. 2010) sub-millime...
Herschel is an ESA space observatory with science instruments provided by European-led Principal Inv...
Context. S-type AGB stars have a C/O ratio which suggests that they are transition objects between o...
Low- and intermediate-mass stars will all eventually enter the asymptotic giant branch (AGB) phase. ...
© ESO 2018. Context. With the outstanding spatial resolution and sensitivity of the Atacama Large Mi...
Context. W Aql is an asymptotic giant branch (AGB) star with an atmospheric elemental abundance rati...
Context. With the outstanding spatial resolution and sensitivity of the Atacama Large Millimeter/sub...
Context. Recent observations at subarcsecond resolution, now possible also at submillimeter waveleng...
[Context] Recent observations at subarcsecond resolution, now possible also at submillimeter wavelen...
Aims. A set of new, sensitive, and spectrally resolved, sub-millimeter line observations are used to...
Herschel is an ESA space observatory with science instruments provided by European-led Principal Inv...
Aims. A set of new, sensitive, and spectrally resolved, sub-millimeter line observations are used to...
Aims. A set of new, sensitive, and spectrally resolved, sub-millimeter line observations are used to...
Aims. A set of new, sensitive, and spectrally resolved, sub-millimeter line observations are used to...
Detailed modelling of the circumstellar molecular line emission of the S-type AGB star W Aquilae
We present new Herschel(1) HIFI (de Graauw et al. 2010) and PACS (Poglitsch et al. 2010) sub-millime...
Herschel is an ESA space observatory with science instruments provided by European-led Principal Inv...
Context. S-type AGB stars have a C/O ratio which suggests that they are transition objects between o...
Low- and intermediate-mass stars will all eventually enter the asymptotic giant branch (AGB) phase. ...
© ESO 2018. Context. With the outstanding spatial resolution and sensitivity of the Atacama Large Mi...
Context. W Aql is an asymptotic giant branch (AGB) star with an atmospheric elemental abundance rati...
Context. With the outstanding spatial resolution and sensitivity of the Atacama Large Millimeter/sub...
Context. Recent observations at subarcsecond resolution, now possible also at submillimeter waveleng...
[Context] Recent observations at subarcsecond resolution, now possible also at submillimeter wavelen...
Aims. A set of new, sensitive, and spectrally resolved, sub-millimeter line observations are used to...
Herschel is an ESA space observatory with science instruments provided by European-led Principal Inv...
Aims. A set of new, sensitive, and spectrally resolved, sub-millimeter line observations are used to...
Aims. A set of new, sensitive, and spectrally resolved, sub-millimeter line observations are used to...
Aims. A set of new, sensitive, and spectrally resolved, sub-millimeter line observations are used to...
Detailed modelling of the circumstellar molecular line emission of the S-type AGB star W Aquilae