Issue |
A&A
Volume 558, October 2013
|
|
---|---|---|
Article Number | A2 | |
Number of page(s) | 7 | |
Section | Stellar structure and evolution | |
DOI | https://doi.org/10.1051/0004-6361/201321883 | |
Published online | 26 September 2013 |
Discovery of a planetary nebula surrounding the symbiotic star DT Serpentis
1
INAF Osservatorio Astronomico di Padova,
36012
Asiago ( VI), Italy
e-mail:
ulisse.munari@oapd.inaf.it
2
Instituto de Astrofisica de Canarias, 38200, La
Laguna, Tenerife, Spain
3
Departamento de Astrofísica, Universidad de La
Laguna, 38206,
La Laguna, Tenerife,
Spain
4
Department of Physics and Astronomy, University of
Padova, 36012
Asiago ( VI), Italy
5
ANS Collaboration, c/o Astronomical Observatory,
36012
Asiago ( VI), Italy
Received: 13 May 2013
Accepted: 11 August 2013
We report the discovery of a planetary nebula centered on the poorly studied symbiotic binary star DT Ser. In a few other symbiotic stars spatially resolved nebulae have been discovered as well, but only one of them probably is a genuine planetary nebula, while the others are likely to originate in complex mass-ejection episodes from the interacting binary central stars that are possibly related to nova-like outbursts. The rim of the planetary nebula around DT Ser is severely distorted toward a brighter star 5 arcsec away. In infrared WISE data, this star shows the presence of a detached cold-dust shell similar to those observed in post-AGB stars. The apparent association of the symbiotic star and its planetary nebula with the nearby possible post-AGB object is discussed. We also discuss the sparse and conflicting literature data that could support an observed variability of the surface brightness of the planetary nebula. The puzzling and intriguing characteristics displayed by DT Ser are surely worth additional and more detailed investigations.
Key words: binaries: symbiotic / planetary nebulae: general / stars: individual: DT Ser / stars: AGB and post-AGB
© ESO, 2013
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.