Detailed studies of IPHAS sources -- III. The highly extinguished bipolar planetary nebula IPHASX J191104.8060845
arXiv:2009.11164 · doi:10.1093/mnras/staa3037
Abstract
We present the first detailed study of the bipolar planetary nebula (PN) IPHASX J191104.8060845 (PN G040.601.5) discovered as part of the Isaac Newton Telescope Photometric H Survey of the Northern Galactic plane (IPHAS). We present Nordic Optical Telescope (NOT) narrow-band images to unveil its true morphology. This PN consists of a main cavity with two newly uncovered extended low-surface brightness lobes located towards the NW and SE directions. Using near-IR WISE images we unveiled the presence of a barrel like structure, which surrounds the main cavity, which would explain the dark lane towards the equatorial regions. We also use Gran Telescopio de Canarias (GTC) spectra to study the physical properties of this PN. We emphasise the potential of old PNe detected in IPHAS to study the final stages of the evolution of the circumstellar medium around solar-like stars.
9 pages, 8 Figures, 3 Tables; Accepted to MNRAS
References in corpus (9)
- An Analysis of the Shapes of Interstellar Extinction Curves. V. The IR-Through-UV Curve Morphology
- Reconstructed Density and Velocity Fields from the 2MASS Redshift Survey
- The Second Data Release of the INT Photometric H-Alpha Survey of the Northern Galactic Plane (IPHAS DR2)
- MASH-II: More Planetary Nebulae from the AAO/UKST HαSurvey
- Do most planetary nebulae derive from binaries? I Population synthesis model of the galactic planetary nebula population produced by singlestars and binaries
- A 3D extinction map of the Northern Galactic Plane based on IPHAS photometry
- Initial Data Release from the INT Photometric H-alpha Survey of the Northern Galactic Plane (IPHAS)
- First release of the IPHAS Catalogue of New Extended Planetary Nebulae
- The Dynamical Evolution of Planetary Nebulae After the Fast Wind