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Characterising Planetary Nebulae in the Large Magellanic Clouds

Published online by Cambridge University Press:  06 October 2025

Silvia Tosi Open the ORCID record for Silvia Tosi [Opens in a new window] ,
Flavia Dell’Agli ,
Devika Kamath ,
Letizia Stanghellini Open the ORCID record for Letizia Stanghellini [Opens in a new window] ,
Paolo Ventura ,
Domingo Aníbal García-Hernández  and
Stefano Bianchi
Silvia Tosi*
Affiliation:
Dipartimento di Matematica e Fisica, Università degli Studi Roma Tre, via della Vasca Navale 84, 00100, Roma, Italy INAF, Osservatorio Astronomico di Roma, Via Frascati 33, 00077, Monte Porzio Catone, Italy Istituto Nazionale di Fisica Nucleare, section of Frascati, Via Enrico Fermi, 54, 00044 Frascati, Italy
Flavia Dell’Agli
Affiliation:
INAF, Osservatorio Astronomico di Roma, Via Frascati 33, 00077, Monte Porzio Catone, Italy
Devika Kamath
Affiliation:
INAF, Osservatorio Astronomico di Roma, Via Frascati 33, 00077, Monte Porzio Catone, Italy Department of Physics and Astronomy, Macquarie University, Sydney, NSW 2109, Australia
Letizia Stanghellini
Affiliation:
NSF’s NOIRLab, 950 Cherry Ave., Tucson, AZ 85719, USA
Paolo Ventura
Affiliation:
INAF, Osservatorio Astronomico di Roma, Via Frascati 33, 00077, Monte Porzio Catone, Italy Istituto Nazionale di Fisica Nucleare, section of Perugia, Via A. Pascoli snc, 06123 Perugia, Italy
Domingo Aníbal García-Hernández
Affiliation:
Instituto de Astrofísica de Canarias (IAC), E-38205 La Laguna, Tenerife, Spain Departamento de Astrofísica, Universidad de La Laguna (ULL), E-38206 La Laguna, Tenerife, Spain
Stefano Bianchi
Affiliation:
Dipartimento di Matematica e Fisica, Università degli Studi Roma Tre, via della Vasca Navale 84, 00100, Roma, Italy
*
email: silvia.tosi@uniroma3.it
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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.

Keywords

planetary nebulaestars: abundances - stars: evolution

Information

Type
Poster Paper
Information
Proceedings of the International Astronomical Union , Volume 19 , Symposium S384: Planetary Nebulae: A Universal Toolbox in the Era of Precision Astrophysics , December 2023 , pp. 394 - 396
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Copyright
© The Author(s), 2025. Published by Cambridge University Press on behalf of International Astronomical Union

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References

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