Optical and Mid-Infrared Observations of the Planetary Nebula NGC 6781
arXiv:1106.3706 · doi:10.1111/j.1365-2966.2011.18722.x
Abstract
Although the planetary nebula NGC 6781 appears to possess an elliptical morphology, its kinematic and emission characteristics are in many ways unusual, and it is possible that it may represent a bipolar source oriented close to the line of sight. We shall present deep imaging of this nebula in [O III], Ha and [N II], and using broad-band (F555W and F814W) filters. These were taken with the 2.56-m Nordic Optical Telescope and Hubble Space Telescope. This is combined with mid-infrared (MIR) imaging and spectroscopy acquired with the Spitzer Space Telescope (Spitzer), and near-infrared spectroscopy deriving from the Infrared Space Observatory (ISO). These reveal details of the complex [N II] structure associated with extended shell emission, perhaps associated with highly inclined bipolar lobes. We also note the presence of narrow absorbing filaments and clumps projected against the surface of the envelope, components which may be responsible for much of the molecular emission. We point out that such clumps may be responsible for complex source structure in the MIR, and give rise to asymmetries in emission along the major axis of the source.
arXiv comment12 pages, 10 figures, Accepted for publication in MNRAS. 32 pages in arXiv
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Cited by in corpus (8)
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- The Herschel Planetary Nebula Survey (HerPlaNS) I. Data Overview and Analysis Demonstration with NGC 6781
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- Extended Structures of Planetary Nebulae Detected in H Emission
- Herschel Planetary Nebula Survey (HerPlaNS) - First Detection of OH+ in Planetary Nebulae
- Spitzer mid-infrared spectroscopic observations of planetary nebulae
- A Herschel study of NGC 650
- The Structure of the Planetary Nebula NGC 2371 in the Visible and Mid-Infrared