Unraveling Disks in AGB Stars
Paper i proceeding, 2015

It is commonly accepted that asymmetries found in the post-AGB stars and planetary nebulae should originate as early as during the AGB phase. We present results from our high-angular resolution observing programs, with an aperture masking technique on the VLT, of a sample of evolved stars that were known to present asymmetries at larger spatial scales (e.g. jets, torii and/or bipolar nebulae). Disk-like structures have been found in the vicinity of at least two of these stars.


F. Lykou

Institut fur Astronomie, Vienna

J. Hron

Institut fur Astronomie, Vienna

A. Zijlstra

Jodrell Bank Centre for Astrophysics

P. G. Tuthill

Sydney Institute for Astronomy

B. R. M. Norris

Sydney Institute for Astronomy

J. Kluska

University of Exeter

C. Paladini

Université libre de Bruxelles (ULB)

E. Lagadec

Observatoire de la Cote d'Azur

M. Wittkowski

European Southern Observatory (ESO)

S. Ramstedt

Uppsala universitet

Matthias Maercker

Chalmers, Rymd- och geovetenskap, Onsala rymdobservatorium

EAS Publications Series

1633-4760 (ISSN) 1638-1963 (eISSN)

Vol. 71-72 217-222
978-2-7598-1907-2 (ISBN)


Astronomi, astrofysik och kosmologi


Grundläggande vetenskaper





Mer information

Senast uppdaterat