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ESO 546-G34 :
ESO 546-G34 : the most-metal-poor, low surface brightness galaxy?
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Mattsson, Lars (författare)
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Pilyugin, Leonid S. (författare)
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- Bergvall, Nils (författare)
- Uppsala universitet,Observationell astrofysik
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(creator_code:org_t)
- 2011-06-07
- 2011
- Engelska.
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Ingår i: Monthly notices of the Royal Astronomical Society. - : Oxford University Press (OUP). - 0035-8711 .- 1365-2966 .- 1745-3925. ; 415:1, s. L54-L58
- Relaterad länk:
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https://academic.oup...
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visa fler...
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https://urn.kb.se/re...
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https://doi.org/10.1...
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Abstract
Ämnesord
Stäng
- We present a re-analysis of spectroscopic data for 23 H(II) regions in 12 blue, metal-poor, low surface brightness galaxies (LSBGs), taking advantage of recent developments in calibrating strong-line methods. In doing so, we have identified a galaxy (ESO 546-G34) which may be the most-metal-poor LSBG found in the local Universe. Furthermore, we find evidence that blue, metal-poor LSBGs, together with blue compact galaxies (BCGs) and many other HII galaxies, fall outside the regular luminosity-metallicity relation. This suggests that there might be an evolutionary connection between LSBGs and BCGs. In such cases, several very metal poor LSBGs should exist in the local Universe.
Ämnesord
- NATURVETENSKAP -- Fysik (hsv//swe)
- NATURAL SCIENCES -- Physical Sciences (hsv//eng)
Nyckelord
- ISM: abundances
- HII regions
- galaxies: dwarf
- galaxies: individual: ESO 546-G34
- Physics
- Fysik
Publikations- och innehållstyp
- ref (ämneskategori)
- art (ämneskategori)
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