PHR 1315−6555: a bipolar planetary nebula in the compact Hyades-age open cluster ESO 96-SC04

@article{Parker2011PHR1A,
  title={PHR 1315−6555: a bipolar planetary nebula in the compact Hyades-age open cluster ESO 96-SC04},
  author={Quentin A. Parker and David J. Frew and Brent Miszalski and Anna V. Kovacevic and Peter M. Frinchaboy and Paul D. Dobbie and J. Taal-Van Koppen},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={2011},
  volume={413},
  pages={1835-1844}
}
We present a detailed study of a bipolar, possible Type I planetary nebula (PN), PHR 1315−6555 (PN G305.3−03.1), which was discovered as part of the Macquarie/AAO/Strasbourg Hα planetary nebula project (MASH), and that we considered at the time was an excellent candidate for membership of the distant, compact, intermediate-age open cluster, ESO 96-SC04. The strong evidence for this association is presented here, making this the only known example of a PN physically associated with a Galactic… 

Figures and Tables from this paper

Further Studies of the Association of Planetary Nebula BMP J16135406 with Galactic Open Cluster NGC 6067
Planetary Nebulae (PNe) that are physical members of Galactic open clusters are powerful probes that allow precise determination of their distance and crucially their initial mass on the main
Hubble Space Telescope Spectroscopy of a Planetary Nebula in an M31 Open Cluster: Hot-bottom Burning at 3.4 M⊙
We use imaging and spectroscopy from the Hubble Space Telescope (HST) to examine the properties of a bright planetary nebula (PN) projected within M31's young open cluster B477-D075. We show that the
A SURVEY FOR PLANETARY NEBULAE IN M31 GLOBULAR CLUSTERS
We report the results of an [O iii] λ5007 spectroscopic survey for planetary nebulae (PNe) located within the star clusters of M31. By examining R ∼ 5000 spectra taken with the WIYN+Hydra
Central Stars of Planetary Nebulae in Galactic Open Clusters: Providing additional data for the White Dwarf Initial-to-Final-Mass Relation
Abstract Accurate (< 10%) distances of Galactic star clusters allow a precise estimation of the physical parameters of any physically associated Planetary Nebula (PN) and also that of its central
Investigating potential planetary nebula/cluster pairs
Context. Fundamental parameters characterizing the end-state of intermediate-mass stars may be constrained by discovering planetary nebulae (PNe) in open clusters (OCs). Cluster membership may be
Planetary Nebulae towards the Galactic bulge – I. [O iii] fluxes
We present [OIII]"5007 fluxes and angular diametres for 435 Planetary Nebulae (PNe) in the central 10 ! "10 ! region towards the Galactic bulge. Our sample is taken from the new discoveries of the
On the crucial cluster Andrews-Lindsay 1 and a 4% distance solution for its planetary nebula
Andrews-Lindsay 1 is a pertinent open cluster because it may host the planetary nebula (PN) PHR 1315-6555, yet ambiguities linger concerning its fundamental parameters (>50% scatter). New multiband
BUBBLES AND KNOTS IN THE KINEMATICAL STRUCTURE OF THE BIPOLAR PLANETARY NEBULA NGC 2818
High-resolution Hubble Space Telescope archive imaging and high-dispersion spectroscopy are used to study the complex morphological and kinematical structure of the planetary nebula, NGC 2818. We
A high-mass planetary nebula in a Galactic open cluster
Planetary nebulae are the ionized ejected envelopes surrounding the remnant cores of dying stars. Theory predicts that main-sequence stars of one to about eight solar masses may eventually form
New light on Galactic post-asymptotic giant branch stars - I. First distance catalogue
We have commenced a detailed analysis of the known sample of Galactic post-asymptotic giant branch (PAGB) objects compiled in the Toru´ n catalogue of Szczerba et al., and present, for the first
...
...

References

SHOWING 1-10 OF 82 REFERENCES
A peculiar planetary nebula candidate in a globular cluster in the Fornax dwarf spheroidal galaxy
Context. Until now, only one planetary nebula (PN) has been known in the Fornax dwarf spheroidal galaxy. Aims. The discovery of a second PN candidate, associated with one of the 5 globular clusters
MASH-II: more planetary nebulae from the AAO/UKST Hα survey
We present a supplement to the Macquarie/AAO/Strasbourg Ha planetary nebulae (PNe) catalogue (MASH), which we denote MASH-II. The supplement consists of over 300 true, likely and possible new
The Macquarie/AAO/Strasbourg Hα Planetary Nebula Catalogue: MASH
We present the Macquarie/AAO/Strasbourg Hα Planetary Nebula Catalogue (MASH) of over 900 true, likely and possible new Galactic planetary nebulae (PNe) discovered from the AAO/UKST Hα survey of the
PFP 1: A Large Planetary Nebula Caught in the First Stages of ISM Interaction
Abstract This paper presents (Hα + [Nii]) imaging and spectroscopy of a previously unknown, highly evolved planetary nebula of low excitation which is in the first stages of an interaction with the
Discovery of an open cluster with a possible physical association with a planetary nebula
We report the discovery of a new open cluster (OC) in the Galaxy at (, =- 167°0 and b = -1°0. Its field includes the planetary nebula (PN) PK 167-0.1. We study the possible associations of the PN/OC
A HUBBLE SPACE TELESCOPE Survey for Resolved Companions of Planetary Nebula Nuclei
We report the results of a Hubble Space Telescope "snapshot" survey aimed at finding resolved binary companions of the central stars of Galactic planetary nebulae (PNe). Using the the Wide Field and
Planetary Nebulae: Observational Properties, Mimics and Diagnostics
  • D. Frew, Q. Parker
  • Physics
    Publications of the Astronomical Society of Australia
  • 2010
Abstract The total number of true, likely and possible planetary nebulae (PN) now known in the Milky Way is nearly 3000, double the number known a decade ago. The new discoveries are a legacy of the
Binary planetary nebulae nuclei towards the Galactic bulge - II. A penchant for bipolarity and low-ionisation structures
Considerable effort has been applied towards understanding the precise shaping mechanisms responsible for the diverse range of morphologies exhibited by planetary nebulae (PNe). At least 10–20% of
Two new evolved bipolar planetary nebulae in the solar neighbourhood
We present AAO/UKST Hα+[N II] narrow-band imagery and low- and medium-resolution optical spectroscopy of RCW 24 and RCW 69. These nebulae were previously classified as H II regions, but we now show
Planetary Nebulae towards the Galactic bulge – I. [O iii] fluxes
We present [OIII]"5007 fluxes and angular diametres for 435 Planetary Nebulae (PNe) in the central 10 ! "10 ! region towards the Galactic bulge. Our sample is taken from the new discoveries of the
...
...