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Star formation and the interstellar medium in low surface brightness galaxies. I. Oxygen abundances and abundance gradients in low surface brightness disk galaxies

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arxiv astro-ph/9803308 v1 pith:5BUQYWTF submitted 1998-03-27 astro-ph

W.J.G. de Blok , J.M. van der Hulst (Kapteyn Astronomical Institute , Groningen , The Netherlands) This is my paper
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keywords oxygenabundancesgalaxiesabundancebrightnessregionssolarsurface
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abstract

We present measurements of the oxygen abundances in 64 HII regions in 12 LSB galaxies. We find that oxygen abundances are low. No regions with solar abundance have been found, and most have oxygen abundances $\sim 0.5$ to 0.1 solar. The oxygen abundance appears to be constant as a function of radius, supporting the picture of quiescently and sporadically evolving LSB galaxies.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. The Merger-Driven Formation of Classical Low Surface Brightness Galaxies in Romulus25

    astro-ph.GA 2025-07 conditional novelty 6.0 of 10

    In the Romulus25 simulation, classical low surface brightness galaxies form mainly through major mergers with aligned, co-rotating orbits that spin up and puff out the remnant galaxy.

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