We have used the SuperCOSMOS Hα Survey to look for faint outer structures such as halos, ansae and jets around known planetary nebulae across 4000 square degrees of the southern Milky Way. Our search will contribute to a more accurate census of these features in the Galactic PN population. Candidate common-envelope PNe have also been identified on the basis of their microstructures. We also intend to determine more reliable distances for these PNe, which should allow a much better statistical basis for the post-AGB total mass budget. Our survey offers fresh scope to address this important issue. © 2012 International Astronomical Union.link_to_subscribed_fulltex
The recent on-line availability of large-scale, wide-field surveys of the Galaxy and Magellanic Clou...
We have developed a method to identify planetary nebula (PN) candidates in imaging data of the Sloan...
Recent Hα surveys such as SHS and IPHAS have improved the completeness of the Galactic planetary neb...
Abstract. We have used the SuperCOSMOS Hα Survey to look for faint outer structures such as halos, a...
Having surveyed ≈ 10% of the sky, we have identified more than 130 PN candidates by surveying multic...
Abstract. The major purpose of this paper is to investi-gate the nature of planetary nebulae (PNe) c...
The AAO/UKST Hα Survey has been used to discover a number of new, large, nearby planetary nebulae (P...
We developed a method to identify planetary nebula (PN) candidates in imaging data of the Sloan...
We present the first results of our search for new, extended planetary nebulae (PNe) based on carefu...
We present the results of a deep and uniform narrowband Hα imaging survey for planetary nebulae (PNs...
Item does not contain fulltextWe present the first results of our search for new, extended planetary...
Using similar to 1700 000 target- and sky-fibre spectra from the Sloan Digital Sky Survey (SDSS), we...
We have extended our planetary nebulae (PNe) survey to the outer ~64 deg2 of the Large Magellanic Cl...
Using ∼ 1,700,000 target- and sky-fiber spectra from the Sloan Digital Sky Survey (SDSS), we have ca...
We have developed a method to identify planetary nebula (PN) candidates in imaging data of the Sloan...
The recent on-line availability of large-scale, wide-field surveys of the Galaxy and Magellanic Clou...
We have developed a method to identify planetary nebula (PN) candidates in imaging data of the Sloan...
Recent Hα surveys such as SHS and IPHAS have improved the completeness of the Galactic planetary neb...
Abstract. We have used the SuperCOSMOS Hα Survey to look for faint outer structures such as halos, a...
Having surveyed ≈ 10% of the sky, we have identified more than 130 PN candidates by surveying multic...
Abstract. The major purpose of this paper is to investi-gate the nature of planetary nebulae (PNe) c...
The AAO/UKST Hα Survey has been used to discover a number of new, large, nearby planetary nebulae (P...
We developed a method to identify planetary nebula (PN) candidates in imaging data of the Sloan...
We present the first results of our search for new, extended planetary nebulae (PNe) based on carefu...
We present the results of a deep and uniform narrowband Hα imaging survey for planetary nebulae (PNs...
Item does not contain fulltextWe present the first results of our search for new, extended planetary...
Using similar to 1700 000 target- and sky-fibre spectra from the Sloan Digital Sky Survey (SDSS), we...
We have extended our planetary nebulae (PNe) survey to the outer ~64 deg2 of the Large Magellanic Cl...
Using ∼ 1,700,000 target- and sky-fiber spectra from the Sloan Digital Sky Survey (SDSS), we have ca...
We have developed a method to identify planetary nebula (PN) candidates in imaging data of the Sloan...
The recent on-line availability of large-scale, wide-field surveys of the Galaxy and Magellanic Clou...
We have developed a method to identify planetary nebula (PN) candidates in imaging data of the Sloan...
Recent Hα surveys such as SHS and IPHAS have improved the completeness of the Galactic planetary neb...