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Article Dans Une Revue Monthly Notices of the Royal Astronomical Society Année : 2011

Ionization of the diffuse gas in galaxies: hot low-mass evolved stars at work

Résumé

We revisit the question of the ionization of the diffuse medium in late-type galaxies, by studying NGC 891, the prototype of edge-on spiral galaxies. The most important challenge for the models considered so far was the observed increase of [O III]/Hbeta, [O II]/Hbeta and [N II]/Halpha with increasing distance to the galactic plane. We propose a scenario based on the expected population of massive OB stars and hot low-mass evolved stars (HOLMES) in this galaxy to explain this observational fact. In the framework of this scenario we construct a finely meshed grid of photoionization models. For each value of the galactic altitude z we look for the models which simultaneously fit the observed values of the [O III]/Hbeta, [O II]/Hbeta and [N II]/Halpha ratios. For each value of z we find a range of solutions which depends on the value of the oxygen abundance. The models which fit the observations indicate a systematic decrease of the electron density with increasing z. They become dominated by the HOLMES with increasing z only when restricting to solar oxygen abundance models, which argues that the metallicity above the galactic plane should be close to solar. They also indicate that N/O increases with increasing z.

Dates et versions

hal-03786225 , version 1 (23-09-2022)

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N. Flores-Fajardo, Christophe Morisset, Grazyna Stasinska, Luc Binette. Ionization of the diffuse gas in galaxies: hot low-mass evolved stars at work. Monthly Notices of the Royal Astronomical Society, 2011, 415, pp.2182-2192. ⟨10.1111/j.1365-2966.2011.18848.x⟩. ⟨hal-03786225⟩
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