Constraining the thermally pulsing asymptotic giant branch phase with resolved stellar populations in the Large Magellanic Cloud

Pastorelli, Giada; Marigo, Paola; Girardi, L.; Aringer, B.; Chen, Yang; Rubele, Stefano; Trabucchi, Michele; Bladh, Sara; L. Boyer, Martha; Bressan, A.; J. Dalcanton, Julianne; A. T. Groenewegen, M.; Lebzelter, T.; Mowlavï, N.; L. Chubb, K.; L. Cioni, Maria-Rosa; de Grijs, Richard; D. Ivanov, V.; Nanni, A.; Th. van Loon, Jacco; Zaggia, S.

doi:10.1093/mnras/staa2565

Public

Constraining the thermally pulsing asymptotic giant branch phase with resolved stellar populations in the Large Magellanic Cloud

Published in Monthly Notices of the Royal Astronomical Society • Aug 20, 2020

Authors:

Giada Pastorelli

Paola Marigo

L. Girardi

Abstract

ABSTRACT Reliable models of the thermally pulsing asymptotic giant branch (TP-AGB) phase are of critical importance across astrophysics, including our interpretation of the spectral energy distribution of galaxies, cosmic dust production, and enrichment of the interstellar medium. With the aim of im...

Subject

Physics

Astrophysics

Asymptotic giant branch

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