Large Magellanic Cloud Planetary Nebula Morphology: Probing Stellar Populations and Evolution.

@article{Stanghellini2000LargeMC,
  title={Large Magellanic Cloud Planetary Nebula Morphology: Probing Stellar Populations and Evolution.},
  author={Stanghellini and Shaw and Balick and Blades},
  journal={The Astrophysical journal},
  year={2000},
  volume={534 2},
  pages={
          L167-L171
        }
}
Planetary nebulae (PNe) in the Large Magellanic Cloud (LMC) offer the unique opportunity to study both the population and evolution of low- and intermediate-mass stars, by means of the morphological type of the nebula. Using observations from our LMC PN morphological survey, and including images available in the Hubble Space Telescope Data Archive and published chemical abundances, we find that asymmetry in PNe is strongly correlated with a younger stellar population, as indicated by the… 
Morphology and Evolution of the Large Magellanic Cloud Planetary Nebulae
The LMC is ideal for studying the coevolution of planetary nebulae (PNs) and their central stars in that the debilitating uncertainties of the Galactic PN distance scale and selection biases from
Recent HST Surveys of Planetary Nebulae in the Magellanic Clouds
The study of the formation and evolution of planetary nebulae (PNs) has been a subject of active investigation for several decades. In the past 15 years the relationship between nebular morphology
The Mass Distribution of the Central Stars of Planetary Nebulae in the Large Magellanic Cloud
We present the properties of the central stars from a sample of 54 planetary nebulae (PNe) observed in the Large Magellanic Cloud (LMC) with the Hubble Space Telescope Imaging Spectrograph (STIS).
Compact Planetary Nebulae in the Galactic Disk: Analysis of the Central Stars
We have obtained multi-wavelength observations of compact Galactic planetary nebulae (PNe) to probe post-Asymptotic Giant Branch (AGB) evolution from the onset of nebular ejection. We analyze new
COMPACT GALACTIC PLANETARY NEBULAE: AN HST/WFC3 MORPHOLOGICAL CATALOG, AND A STUDY OF THEIR ROLE IN THE GALAXY
We present the images of a Hubble Space Telescope (HST/WFC3) snapshot program of angularly compact Galactic planetary nebulae (PNe), acquired with the aim of studying their size, evolutionary status,
A test for asymptotic giant branch evolution theories: Planetary Nebulae in the Large Magellanic Cloud
We used a new generation of asymptotic giant branch (AGB) stellar models that include dust formation in the stellar winds to find the links between evolutionary models and the observed properties of
The Large Magellanic Cloud PN population
  • W. Reid
  • Physics
    Proceedings of the International Astronomical Union
  • 2015
Abstract The Large Magellanic Cloud (LMC) and Small Magellanic Cloud (SMC) allow us to study late stellar evolution in environments that are respectively about a half and a quarter the metallicity of
AGB Stars and the Observed Abundance of Neon in Planetary Nebulae
Abstract Asymptotic giant branch stars are expected to produce 22Ne through the combined H and He burning that operates during their thermally pulsing evolution. However, observationally there is a
Spherical planetary nebulae
By examining their mass loss history and their distribution in the galaxy, I argue that spherical planetary nebulae (PNe) form a special group among all planetary nebulae. The smooth surface
Planetary nebulae in the Magellanic Clouds , II. Abundances and element production
Context. We present the second part of an optical spectroscopic study of planetary nebulae in the LMC and SMC. The first paper, Leisy & Dennefeld (1996, A&AS, 116, 96), discussed the CNO cycle for
...
1
2
3
...

References

SHOWING 1-10 OF 16 REFERENCES
Photoionization modeling of Magellanic Cloud planetary nebulae. I
The results of self-consistent photoionization modeling of 38 Magellanic Cloud PNe are presented and used to construct an H-R diagram for the central stars and to obtain both the nebular chemical
Hubble Space Telescope Images of Magellanic Cloud Planetary Nebulae: Data and Correlations across Morphological Classes*
The morphology of planetary nebulae (PNs) provides an essential tool for understanding their origin and evolution, since it reflects both the dynamics of the gas ejected at the tip of the asymptotic
Hubble Space Telescope Observations of Planetary Nebulae in the Magellanic Clouds. V. Mass Dependence of Dredge-up and the Chemical History of the Large Magellanic Cloud
A photoionization analysis of Hubble Space Telescope UV and ground-based optical spectrophotometry is given for eight more planetary nebulae (PNs) in the Large Magellanic Cloud (LMC). This allows the
Abundances of the heavy elements in the Magellanic Clouds. II - H II regions and supernova remnants
The first consistent abundance analysis of both H II regions and SNRs in the Magellanic Clouds is presented. Detailed modeling of the SNRs results in abundance measures in good agreement with those
Nebular Abundance Errors.
The errors inherent to the use of the standard "ionization correction factor" ("i_CF") method of calculating nebular conditions and relative abundances of H, He, N, O, Ne, S, and Ar in emission line
New theoretical yields of intermediate mass stars
TLDR
The abundances predicted during the nal stages of the AGB with those observed in planetary nebu- lae in the Galactic disk are compared and show that the model with the aforementioned parameters is in good agreement with the observations.
Astrophysics of Gaseous Nebulae and Active Galactic Nuclei
Preface Preface to First Edition General Introduction Photoionization Equilibrium Thermal Equilibrium Calculation of Emitted Spectrum Comparison of Theory with Observations Internal Dynamics of
Planetary Nebulae of Type I Revisited
Type I PNe were defined in 1977; during the last 19 years evidence has accumulated indicating that indeed these objects form a distinct physical group, corresponding to the high mass end of the
Spectral Classification of Emission-Line Galaxies
A revised method of classification of narrow-line active galaxies and H II region-like galaxies is proposed. It involves the line ratios which take full advantage of the physical distinction between
An optical spectrophotometric survey of abundances in Magellanic Cloud Planetary Nebulae
Analyse des abondances pour 71 nebuleuses planetaires dans le Grand et Petit Nuage de Magellan a partir de donnees de spectroscopie optique
...
1
2
...