Abstract
The butterfly-shaped planetary nebula, NGC 6302, shows a dense equatorial dark lane, which is presumably a dusty disc. We report observations of the dark lane based on Hubble Space Telescope (HST) Hα image, James Clerk Maxwell Telescope (JCMT) 450 μm images, and JCMT 12CO, 13CO J=2-1 and 3-2 line observations. © 2005 American Institute of Physics.
| Original language | English |
|---|---|
| Title of host publication | AIP Conference Proceedings|AIP Conf. Proc. |
| Pages | 211 |
| Volume | 804 |
| DOIs | |
| Publication status | Published - 28 Nov 2005 |
| Event | International Conference on Planetary Nebulae as Astronomical Tools - Gdansk Duration: 28 Nov 2005 → … |
Conference
| Conference | International Conference on Planetary Nebulae as Astronomical Tools |
|---|---|
| City | Gdansk |
| Period | 28/11/05 → … |
Keywords
- (ISM:)dust, extinction
- (ISM:)Planetary nebulae:individual:NGC 6302
- ISM: jets and outflows
Fingerprint
Dive into the research topics of 'The dark lane of the bipolar nebula NGC 6302'. Together they form a unique fingerprint.Cite this
- APA
- Author
- BIBTEX
- Harvard
- Standard
- RIS
- Vancouver