On the Age of Galactic Bulge CSPNe: Too Young and Complicated?

We present preliminary results of our study of a small sample of planetary nebulae in the Galactic Bulge for which high-angular resolution Hubble Space Telescope imaging is available. From this and from archival spectroscopy, we were able to calculate temperatures and luminosities for their central...

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Main Authors: Foteini Lykou, Albert Zijlstra, Quentin A. Parker
Format: Article
Language:English
Published: MDPI AG 2020-06-01
Series:Galaxies
Subjects:
Online Access:https://www.mdpi.com/2075-4434/8/2/51
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author Foteini Lykou
Albert Zijlstra
Quentin A. Parker
author_facet Foteini Lykou
Albert Zijlstra
Quentin A. Parker
author_sort Foteini Lykou
collection DOAJ
description We present preliminary results of our study of a small sample of planetary nebulae in the Galactic Bulge for which high-angular resolution Hubble Space Telescope imaging is available. From this and from archival spectroscopy, we were able to calculate temperatures and luminosities for their central stars. These were then correlated to up-to-date evolutionary tracks found in the literature to help us estimate stellar masses and therefore ages for the central stars. Our current analysis indicates that our sample appears to represent a somewhat mixed population of planetary nebulae central stars, while at least one of the nebulae might have been formed by a more massive progenitor (i.e., <inline-formula> <math display="inline"> <semantics> <mrow> <msub> <mi>M</mi> <mi>ZAMS</mi> </msub> <mo>∼</mo> <mn>4</mn> </mrow> </semantics> </math> </inline-formula> M<inline-formula> <math display="inline"> <semantics> <msub> <mrow></mrow> <mo>⊙</mo> </msub> </semantics> </math> </inline-formula>).
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spelling doaj.art-b5467130db804fa7a93b8263c2fe2fad2023-11-20T04:14:14ZengMDPI AGGalaxies2075-44342020-06-01825110.3390/galaxies8020051On the Age of Galactic Bulge CSPNe: Too Young and Complicated?Foteini Lykou0Albert Zijlstra1Quentin A. Parker2Department of Physics, C.Y.M. Physics Building, The University of Hong Kong, Pokfulam Road, Hong Kong, ChinaLaboratory for Space Research, The University of Hong Kong, Block A, Cyberport 4, 100 Cyberport Rd, Cyberport, Hong Kong, ChinaDepartment of Physics, C.Y.M. Physics Building, The University of Hong Kong, Pokfulam Road, Hong Kong, ChinaWe present preliminary results of our study of a small sample of planetary nebulae in the Galactic Bulge for which high-angular resolution Hubble Space Telescope imaging is available. From this and from archival spectroscopy, we were able to calculate temperatures and luminosities for their central stars. These were then correlated to up-to-date evolutionary tracks found in the literature to help us estimate stellar masses and therefore ages for the central stars. Our current analysis indicates that our sample appears to represent a somewhat mixed population of planetary nebulae central stars, while at least one of the nebulae might have been formed by a more massive progenitor (i.e., <inline-formula> <math display="inline"> <semantics> <mrow> <msub> <mi>M</mi> <mi>ZAMS</mi> </msub> <mo>∼</mo> <mn>4</mn> </mrow> </semantics> </math> </inline-formula> M<inline-formula> <math display="inline"> <semantics> <msub> <mrow></mrow> <mo>⊙</mo> </msub> </semantics> </math> </inline-formula>).https://www.mdpi.com/2075-4434/8/2/51planetary nebulaewhite dwarfsstellar evolution
spellingShingle Foteini Lykou
Albert Zijlstra
Quentin A. Parker
On the Age of Galactic Bulge CSPNe: Too Young and Complicated?
Galaxies
planetary nebulae
white dwarfs
stellar evolution
title On the Age of Galactic Bulge CSPNe: Too Young and Complicated?
title_full On the Age of Galactic Bulge CSPNe: Too Young and Complicated?
title_fullStr On the Age of Galactic Bulge CSPNe: Too Young and Complicated?
title_full_unstemmed On the Age of Galactic Bulge CSPNe: Too Young and Complicated?
title_short On the Age of Galactic Bulge CSPNe: Too Young and Complicated?
title_sort on the age of galactic bulge cspne too young and complicated
topic planetary nebulae
white dwarfs
stellar evolution
url https://www.mdpi.com/2075-4434/8/2/51
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