期刊
ASTRONOMY & ASTROPHYSICS
卷 539, 期 -, 页码 -出版社
EDP SCIENCES S A
DOI: 10.1051/0004-6361/201117923
关键词
planetary nebulae: general; planetary nebulae: individual: NGC 6778; ISM: jets and outflows; binaries: close
资金
- Spanish MICINN [AYA2008-01934, AYA2011-29754-C03-02]
- FEDER
- Xunta de Galicia [INCITE09 E1R312096, INCITE09 312191PR, IN8458-2010/061]
The planetary nebula (PN) NGC 6778 harbors a binary central star with a short orbital period and displays two systems of fast collimated outflows. To assess the influence of the evolution through a common-envelope phase of the binary system of NGC 6778 on its formation and shaping, we have used narrow-band images and high-dispersion long-slit spectra of the nebula to investigate its detailed morphology and kinematics. We find that the overall structure of NGC 6778 can be described as a bipolar PN. The equatorial ring is highly disrupted and many radial features (filamentary wisps and cometary knots) also show strong dynamical effects. There are clear connections between the bipolar lobes and the fast collimated outflows: the collimated outflows seem to arise from bright knots at the tips of the bipolar lobes, whereas the kinematics of the bipolar lobes is distorted. We suggest that the interaction of the fast collimated outflows of NGC 6778 with its nebular envelope has resulted in the disruption of the nebular shell and equatorial ring.
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