October 8, 2025

Characterising Planetary Nebulae in the Large Magellanic Clouds

Key Points

The study reveals new insights into the dust contribution in planetary nebulae, emphasizing their importance in stellar evolution.
Observations ranged from UV to IR, allowing a detailed analysis of 10 planetary nebulae in the Large Magellanic Cloud.
Characterization of the central stars was linked to the historical evolution of these low- and intermediate-mass stellar sources.
Findings provide foundational data for understanding the gas and dust enrichment in the universe.

Abstract

Abstract Planetary nebulae (PNe) represent the final link in the chain of the gas and dust enrichment of low- and intermediate-mass stars. We present a comprehensive study of the relevant observational data of 10 PNe of the Large Magellanic Cloud (LMC). Analysing them from the UV to the IR, we characterise the nature of the central star (CS) and the dust contribution. We link these results to the evolutionary history of these sources.

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Discussion

Authors

S. Tosi

F. Dell’Agli

D. Kamath

Journals

Proceedings of the International Astronomical Union

Actions

Institutions

Macquarie University

Universidad de La Laguna

Roma Tre University

References and Citations

Connected Papers

Building similarity graph...

Analyzing shared references across papers

Characterising Planetary Nebulae in the Large Magellanic Clouds

Key Points

Abstract

Citation Network

Connected Papers

Discussion

Authors

Journals

Actions

Institutions

References and Citations

Citation Network

Connected Papers

Discussion

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