Discovery of metal-poor and distant pre-main sequence candidates in WLM with JWST

Fuente: arXiv
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Autores principales: Kalari, Venu M., Salinas, Ricardo, Andersen, Morten, De Marchi, Guido, Rubio, Monica, Vink, Jorick S., Zinnecker, Hans
Formato: Preprint
Publicado: 2025
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author Kalari, Venu M.
Salinas, Ricardo
Andersen, Morten
De Marchi, Guido
Rubio, Monica
Vink, Jorick S.
Zinnecker, Hans
author_facet Kalari, Venu M.
Salinas, Ricardo
Andersen, Morten
De Marchi, Guido
Rubio, Monica
Vink, Jorick S.
Zinnecker, Hans
contents We present the discovery of twelve metal-poor and distant pre-main sequence (PMS) candidates in the dwarf irregular galaxy Wolf-Lundmark-Melotte (WLM)~968 kpc away, at a present-day metallicity of [Fe/H] around $-$0.9. These candidates have masses between 1.25-5 M$_{\odot}$, with ages <10 Myr, and exhibit significant near-infrared excesses at 2.5 and 4.3 $μ$m. They are concentrated within a cluster roughly 10 pc (2'') across situated in the HII region [HM95]-9. These are the most distant and metal-poor PMS stars known, and can offer new quantitative insights into star formation at low-metallicities.
format Preprint
id arxiv_https___arxiv_org_abs_2501_17097
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Discovery of metal-poor and distant pre-main sequence candidates in WLM with JWST
Kalari, Venu M.
Salinas, Ricardo
Andersen, Morten
De Marchi, Guido
Rubio, Monica
Vink, Jorick S.
Zinnecker, Hans
Solar and Stellar Astrophysics
Astrophysics of Galaxies
We present the discovery of twelve metal-poor and distant pre-main sequence (PMS) candidates in the dwarf irregular galaxy Wolf-Lundmark-Melotte (WLM)~968 kpc away, at a present-day metallicity of [Fe/H] around $-$0.9. These candidates have masses between 1.25-5 M$_{\odot}$, with ages <10 Myr, and exhibit significant near-infrared excesses at 2.5 and 4.3 $μ$m. They are concentrated within a cluster roughly 10 pc (2'') across situated in the HII region [HM95]-9. These are the most distant and metal-poor PMS stars known, and can offer new quantitative insights into star formation at low-metallicities.
title Discovery of metal-poor and distant pre-main sequence candidates in WLM with JWST
topic Solar and Stellar Astrophysics
Astrophysics of Galaxies
url https://arxiv.org/abs/2501.17097