First deep images catalogue of extended IPHAS PNe

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 pur...

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Detalles Bibliográficos
Autores: Sabin, L., Guerrero, Martín A., Ramos-Larios, G., Boumis, P., Zijlstra, Albert, Awang Iskandar, D. N. F., Barlow, M. J., Toalá, Jesús A., Parker, Quentin A., Corradi, R. M. L., Morris, R. A. H.
Tipo de recurso: artículo
Estado:Versión publicada
Fecha de publicación:2021
País:España
Institución:Consejo Superior de Investigaciones Científicas (CSIC)
Repositorio:DIGITAL.CSIC. Repositorio Institucional del CSIC
OAI Identifier:oai:dnet:digitalcsic_::be4e318b8c144567799cfce9bd186a6f
Acceso en línea:http://hdl.handle.net/10261/260440
Access Level:acceso abierto
Palabra clave:Stars: mass-loss
Stars: winds
Outflows
Planetary nebulae
Descripción
Sumario: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. © 2021 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society.