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Abstract
We report on the observations of the circumstellar envelope of the AGB star II Lup in the near- and mid-infrared with the use of direct imaging and interferometric techniques. Our findings indicate that the circumstellar envelope is not spherically symmetric and that the majority of the emission originates within 0.5 arcsec from the star.
Original language | English |
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Article number | 108 |
Journal | Galaxies |
Volume | 6 |
Issue number | 4 |
Early online date | 12 Oct 2018 |
DOIs | |
Publication status | Published - 2018 |
Keywords
- AGB stars
- Aperture masking
- Infrared interferometry
- Observations
- Stellar evolution
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Dive into the research topics of 'Infrared observations of the asymmetric mass loss of an AGB star'. Together they form a unique fingerprint.Activities
- 1 Visiting an external academic institution
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University of Hong Kong
Zijlstra, A. (Secondee)
1 May 2018 → 15 Jun 2018Activity: External visiting positions or secondments › Visiting an external academic institution › Research