Published in

MDPI, Galaxies, 4(6), p. 108, 2018

DOI: 10.3390/galaxies6040108

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Infrared Observations of the Asymmetric Mass Loss of an AGB Star

This paper is made freely available by the publisher.
This paper is made freely available by the publisher.

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Data provided by SHERPA/RoMEO

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.

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