Abstract
We present the first instalment of a deep imaging catalogue containing
58 True, Likely, and Possible extended PNe detected with the Isaac
Newton Telescope Photometric H α Survey (IPHAS). The three
narrow-band filters in the emission lines of H α, [N II]
λ6584 Å, and [O III] λ5007 Å used for this
purpose allowed us to improve our description of the morphology and
dimensions of the nebulae. In some cases even the nature of the source
has been reassessed. We were then able to unveil new macro- and
micro-structures, which will without a doubt contribute to a more
accurate analysis of these PNe. It has been also possible to perform a
primary classification of the targets based on their ionization level. A
Deep Learning classification tool has also been tested. We expect that
all the PNe from the IPHAS catalogue of new extended planetary nebulae
will ultimately be part of this deep H α, [N II], and [O III]
imaging catalogue.
Original language | English |
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Pages (from-to) | 1599–1617 |
Number of pages | 19 |
Journal | Monthly Notices of the Royal Astronomical Society |
Volume | 508 |
Issue number | 2 |
Early online date | 21 Sept 2021 |
DOIs | |
Publication status | Published - 31 Dec 2021 |
Bibliographical note
Publisher Copyright:© 2021 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society.
Keywords
- stars: mass-loss
- stars: winds
- outflows
- planetary nebulae