dorsal/arxiv
View SchemaFirst direct electron temperature measurement in [O II] zone in I Zw 18
| Authors | I. A. Zinchenko, J. M. Vílchez, C. Kehrig, P. Papaderos, J. E. Méndez-Delgado |
|---|---|
| Categories | |
| ArXiv ID | 2601.08722vv1 |
| URL | https://arxiv.org/abs/2601.08722 |
| License | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ |
Abstract
We present new precise measurements of electron temperatures and oxygen abundances in the southeast knot of I Zw 18, one of the most metal-poor blue compact dwarf galaxies known, using spectroscopic data from the Dark Energy Spectroscopic Instrument Data Release 1 (DESI DR1). For the first time in I Zw 18, we directly measure electron temperature in the low-ionization zone using the rarely detected [O II] $\lambda\lambda7320,7330$ doublet. We also detect the auroral lines [O III] $\lambda4363$ and [S III] $\lambda6312$, associated with high and intermediate ionization zones, respectively. We derive $T_{\mathrm{e}}([\mathrm{O}\,\mathrm{III}])=21\,200\pm860\ \mathrm{K}$, $T_{\mathrm{e}}([\mathrm{O}\,\mathrm{II}])=16\,170\pm950\ \mathrm{K}$, and $T_{\mathrm{e}}([\mathrm{S}\,\mathrm{III}])=17\,290\pm1750\ \mathrm{K}$, highlighting a significant temperature difference between ionization zones. Using these direct temperature measurements, we determine a total oxygen abundance of $12+\log(\mathrm{O}/\mathrm{H})=7.066\pm0.046$, $\log(\mathrm{N}/\mathrm{O})=-1.509\pm0.097$, and $\log(\mathrm{S}/\mathrm{O})=-1.558\pm0.041$. Our results extend the calibration of $t_2$--$t_3$ relations to the highest temperatures, providing important anchor points for the temperature structure of extremely metal-poor H II regions, including high-redshift galaxies where direct temperature measurements are especially challenging.
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"date_created": "2026-02-17T05:53:15.712000Z",
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"abstract": "We present new precise measurements of electron temperatures and oxygen abundances in the southeast knot of I Zw 18, one of the most metal-poor blue compact dwarf galaxies known, using spectroscopic data from the Dark Energy Spectroscopic Instrument Data Release 1 (DESI DR1). For the first time in I Zw 18, we directly measure electron temperature in the low-ionization zone using the rarely detected [O II] $\\lambda\\lambda7320,7330$ doublet. We also detect the auroral lines [O III] $\\lambda4363$ and [S III] $\\lambda6312$, associated with high and intermediate ionization zones, respectively. We derive $T_{\\mathrm{e}}([\\mathrm{O}\\,\\mathrm{III}])=21\\,200\\pm860\\ \\mathrm{K}$, $T_{\\mathrm{e}}([\\mathrm{O}\\,\\mathrm{II}])=16\\,170\\pm950\\ \\mathrm{K}$, and $T_{\\mathrm{e}}([\\mathrm{S}\\,\\mathrm{III}])=17\\,290\\pm1750\\ \\mathrm{K}$, highlighting a significant temperature difference between ionization zones. Using these direct temperature measurements, we determine a total oxygen abundance of $12+\\log(\\mathrm{O}/\\mathrm{H})=7.066\\pm0.046$, $\\log(\\mathrm{N}/\\mathrm{O})=-1.509\\pm0.097$, and $\\log(\\mathrm{S}/\\mathrm{O})=-1.558\\pm0.041$. Our results extend the calibration of $t_2$--$t_3$ relations to the highest temperatures, providing important anchor points for the temperature structure of extremely metal-poor H II regions, including high-redshift galaxies where direct temperature measurements are especially challenging.",
"arxiv_id": "2601.08722",
"authors": [
"I. A. Zinchenko",
"J. M. V\u00edlchez",
"C. Kehrig",
"P. Papaderos",
"J. E. M\u00e9ndez-Delgado"
],
"categories": [
"astro-ph.GA"
],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"title": "First direct electron temperature measurement in [O II] zone in I Zw 18",
"url": "https://arxiv.org/abs/2601.08722",
"version": "v1"
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