1. Metals and dust content across the galaxies M101 and NGC628
- Author
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I. De Looze, Monica Relano, José M. Vílchez, M. Mollá, Maud Galametz, Robert C. Kennicutt, Ministerio de Economía y Competitividad (España), Junta de Andalucía, European Commission, Kennicutt, Robert [0000-0001-5448-1821], and Apollo - University of Cambridge Repository
- Subjects
Dust,extinction ,Extinction – ISM ,Galaxies: abundances ,astro-ph.GA ,FOS: Physical sciences ,CHEMICAL EVOLUTION ,Individual ,Astrophysics::Cosmology and Extragalactic Astrophysics ,Abundances – galaxies ,01 natural sciences ,individual: NGC 5457 and NGC 628 [galaxies] ,H-II REGIONS ,Regional development ,0103 physical sciences ,abundances [galaxies] ,STAR-FORMING GALAXIES ,Astrophysics::Solar and Stellar Astrophysics ,NEARBY GALAXIES ,INTEGRAL FIELD SPECTROSCOPY ,010303 astronomy & astrophysics ,Astrophysics::Galaxy Astrophysics ,molecules [ISM] ,Luminosity function (astronomy) ,Physics ,Spiral galaxy ,ISM [galaxies] ,010308 nuclear & particles physics ,extinction ,METALLICITY RELATION ,Astronomy and Astrophysics ,Dust ,Astrophysics - Astrophysics of Galaxies ,ISM: molecules ,Galaxy ,OXYGEN ABUNDANCE ,Chemical evolution ,Galaxies: ISM ,Molecules – galaxies ,Physics and Astronomy ,Space and Planetary Science ,LUMINOSITY FUNCTION ,Astrophysics of Galaxies (astro-ph.GA) ,Galaxies: individual: NGC 5457 and NGC 628 ,Astrophysics::Earth and Planetary Astrophysics ,Humanities ,SPIRAL GALAXIES ,INTERSTELLAR DUST - Abstract
We present a spatially resolved study of the relation between dust and metallicity in the nearby spiral galaxies M 101 (NGC 5457) and NGC 628 (M 74). We explore the relation between the chemical abundances of their gas and stars with their dust content and their chemical evolution. The empirical spatially resolved oxygen effective yield and the gas-to-dust mass ratio (GDR) across both disc galaxies are derived, sampling 1 dex in oxygen abundance. We find that the metal budget of the NGC 628 disc and most of the M 101 disc appears consistent with the predictions of the simple model of chemical evolution for an oxygen yield between half and one solar, whereas the outermost region (R ≥ 0.8 R 25 ) of M 101 presents deviations suggesting the presence of gas flows. The GDR-metallicity relation shows a two slopes behaviour, with a break at 12 + log(O/H) ≈ 8.4, a critical metallicity predicted by theoretical dust models when stardust production equals grain growth. A relation between GDR and the fraction of molecular to total gas, ΣH 2 }/Σ gas is also found. We suggest an empirical relationship between GDR and the combination of 12 + log(O/H), for metallicity, and ΣH 2 /Σ gas , a proxy for the molecular clouds fraction. The GDR is closely related with metallicity at low abundance and with ΣH 2 /Σ gas for higher metallicities suggesting interstellar medium dust growth. The ratio Σ dust /Σ star correlates well with 12+ log(O/H) and strongly with log(N/O) in both galaxies. For abundances below the critical one, the 'stardust' production gives us a constant value suggesting a stellar dust yield similar to the oxygen yield. © 2018 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society., This work was partially supported by the Spanish Ministerio de Economia y Competitividad under grants AYA2016-79724-C4-4-P and AYA2016-79724-C4-3-P, and excellence project PEX2011-FQM-7058 of Junta de Andalucia (Spain). MR acknowledges support by the research projects AYA2014-53506-P and AYA2017-84897-P from the Spanish Ministerio de Economia y Competitividad and Junta de Andalucia grant FQM108; support from the European Regional Development Funds (FEDER) is acknowledged.
- Published
- 2018