A new population of planetary nebulae candidates towards the Galactic bulge

T. N. Stenborg, Q. A. Parker

Research output: Chapter in Book/Report/Conference proceedingConference proceeding contribution

Abstract

We discuss discovery of a new population of up to 300 planetary nebulae (PNe) candidates captured serendipitously in deep [OIII] imaging of the Galactic Bulge taken with the Mosaic II wide-field CCD imager on the Cerro Tololo Inter-American Observatory's 4 m Blanco telescope. This imaging was taken to determine accurate [OIII] fluxes for known Bulge PNe, but, through careful examination, is also yielding significant numbers of new PNe candidates. These new candidates range from compact but still relatively faint sources, through to very extended, low surface brightness PNe. The new population is summarised, discovery techniques reviewed and preliminary confirmatory spectroscopy presented. Implications for the PNe bulge population and luminosity function are briefly discussed.
Original languageEnglish
Title of host publicationAsymmetrical Planetary Nebulae VI
Subtitle of host publicationproceedings
EditorsC. Morisset, G. Delgado-Inglada, S. Torres-Peimbert
Place of PublicationRiviera Maya, Mexico
PublisherProceedings of the Asymmetrical Planetary Nebulae VI conference
Pages1
Number of pages1
Publication statusPublished - 2014
EventAsymmetrical Planetary Nebulae (6th : 2013) - Riviera Maya, Mexico
Duration: 4 Nov 20138 Nov 2013

Conference

ConferenceAsymmetrical Planetary Nebulae (6th : 2013)
CityRiviera Maya, Mexico
Period4/11/138/11/13

Keywords

  • stars: planetary nebulae
  • planetary nebulae: general

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