The Mass-to-Light Ratios of Spiral Disks

Ciardullo, Robin; Herrmann, Kimberly A.

doi:10.1007/978-1-4020-6933-8_32

Cited by 1 publication

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“…The snapshot survey targets plotted in Figures 5 and 6 were selected from the brightest LMC and SMC PNe [4,5], thus the completeness near the high luminosity cut-off should be adequate [17]. In both Figures, but more clearly in Figure 5, one can see two different branches of PNe, running from small to large radii.…”

Section: The Planetary Nebula Lumonsity Functionmentioning

confidence: 99%

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Clues on Post-Asymptotic Giant Branch Evolution and Planetary Nebulae Populations from the Magellanic Clouds

Stanghellini

Planetary Nebulae Beyond the Milky Way

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Abstract.The recent HST optical images, and the optical and ultraviolet spectra, of Magellanic planetary nebulae (PNe), together with the large data-base that has been collected in the past decade, allows unprecedented insight in the evolution of PNe and their central stars. In this paper we present a selection of recent results: The analysis of PN morphology, both in the optical and ultra-violet emission lines; the relation between nebular morphology and the chemistry produced by stellar evolution; the direct determination of the transition time from observations; and the study of the nature and evolutionary stage of the components of the planetary nebula luminosity function.

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Section: The Planetary Nebula Lumonsity Functionmentioning

confidence: 99%

“…The planetary nebula luminosity function (PNLF) is a well-known secondary distance indicator [17]. The high-luminosity cut-off of the PNLF seems to be invariant for galaxies with similar metallicites, while with a metallicity-correction it is also possible to unify the method for all galaxies.…”

Section: The Planetary Nebula Lumonsity Functionmentioning

confidence: 99%

Clues on Post-Asymptotic Giant Branch Evolution and Planetary Nebulae Populations from the Magellanic Clouds

Stanghellini

Planetary Nebulae Beyond the Milky Way

View full text Add to dashboard Cite

show abstract

The Mass-to-Light Ratios of Spiral Disks

Cited by 1 publication

References 7 publications

Clues on Post-Asymptotic Giant Branch Evolution and Planetary Nebulae Populations from the Magellanic Clouds

Clues on Post-Asymptotic Giant Branch Evolution and Planetary Nebulae Populations from the Magellanic Clouds

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