The “Príncipes de Asturias” nebula: a new quadrupolar planetary nebula from the IPHAS survey
Instituto de Astrofísica de Canarias, 38200 La Laguna, Tenerife, Spain e-mail: email@example.com; firstname.lastname@example.org
2 Isaac Newton Group. Ap. de Correos 321, 38700 Sta. Cruz de la Palma, Spain e-mail: [rcorradi;pleisy;greimel]@ing.iac.es
3 Imperial College, Blackett Laboratory, Exhibition Road, London, SW7 2AZ, UK e-mail: email@example.com
4 University College London. Department of Physics and Astronomy. Gower St. London WC1E 6BT, UK e-mail: firstname.lastname@example.org
5 Department of Physics, Macquarie University, NSW 2109, Australia e-mail: [dfrew;qap]@ics.mq.edu.au
6 Cambridge Astronomical Survey Unit, Institute of Astronomy, Cambridge, UK e-mail: email@example.com
7 Astrophysics Group, Department of Physics, Bristol University, Tyndall Avenue, Bristol, BS8 1TL, UK e-mail: [r.morris;s.phillipps]@bristol.ac.uk
8 Instituto de Geofísica y Astronomía. Calle 212, No. 2906, CP 11600, La Habana, Cuba e-mail: firstname.lastname@example.org
9 School of Physics and Astronomy, Manchester Univ., Sackville Street, PO Box 88, Manchester M60 1QD, UK e-mail: email@example.com
Accepted: 10 July 2006
Context.The Isaac Newton Telescope Photometric Hα Survey (IPHAS) is currently mapping the Northern Galactic plane reaching to mag with typically 1″ resolution. Hundreds of Planetary Nebulae (PNe), both point-like and resolved, are expected to be discovered. We report on the discovery of the first new PN from this survey: it is an unusual object located at a large galactocentric distance and has a very low oxygen abundance.
Aims.Detecting and studying new PNe will lead to improved estimates of the population size, binary fraction and lifetimes, and yield new insights into the chemistry of the interstellar medium at large galactocentric distances.
Methods.Compact nebulae are searched for in the IPHAS photometric catalogue, selecting those candidates with a strong Hα excess in the vs. colour–colour diagram. Searches for extended nebulae are by visual inspection of the mosaics of continuum-subtracted Hα images at a spatial sampling of arcsec2. Follow-up spectroscopy enables confirmation of the PNe, and their physico-chemical study.
Results.The first planetary nebula discovered via IPHAS imagery shows an intricate morphology: there is an inner ring surrounding the central star, bright inner lobes with an enhanced waist, and very faint lobular extensions reaching up to more than 100''. We classify it as a quadrupolar PN, a rather unusual class of planetary showing two pairs of misaligned lobes. From long-slit spectroscopy we derive Te[ Nii K, cm-3, and chemical abundances typical of Peimbert's type I nebulae (, ) with an oxygen abundance of . A kinematic distance of 7.0 kpc is derived, implying an unusually large size of >4 pc for the nebula. The photometry of the central star indicates the presence of a relatively cool companion. This, and the evidence for a dense circumstellar disk and quadrupolar morphology, all of which are rare among PNe, support the hypothesis that this morphology is related to binary interaction.
Key words: planetary nebulae: general / ISM: abundances
© ESO, 2006