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Iron Depletion in ionized Nebulae of the Large Magellanic Cloud

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arxiv 1103.2158 v1 pith:3E4WA7MX submitted 2011-03-10 astro-ph.SR astro-ph.CO

G. Delgado-Inglada , M. Rodríguez , J. García-Rojas , M. Peña , M. T. Ruiz This is my paper · ORCID
classification astro-ph.SRastro-ph.CO
keywords nebulaeironclouddepletiongalacticionizedlargelower
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We present here preliminary results of an analysis of the iron abundance in the ionized gas of three planetary nebulae and one H II region of the Large Magellanic Cloud (LMC). These results are compared with the ones we obtain for a sample of Galactic and extragalactic nebulae. We find that the amounts of iron depletion into dust grains in LMC nebulae are similar to those found in Galactic nebulae. Objects with lower metallicities show lower depletions, but a larger sample of objects is needed to explore the reasons behind this trend.

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  1. Observing Co-Located Neutral and Ionized Gas-Phase Iron Depletion in the Magellanic Clouds

    astro-ph.GA 2026-08 conditional novelty 6.0 of 10

    H II regions in the Magellanic Clouds can have lower gas-phase iron abundances than co-located neutral gas, indicating stronger iron depletion into dust.

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