Mass-metallicity relation explored with CALIFA I. Is there a dependence on the star-formation rate?
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474 citations
Cites background or methods or result from "Mass-metallicity relation explored ..."
...Z relation (e.g., Tremonti et al. 2004; Sanchez et al. 2013)....
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...Since the representative abundance (i.e., the abundance at the disk effective radius) scales with the integrated mass (Sanchez et al. 2013) following the well knownM–...
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...Z relation Rosales-Ortega et al. (2012); Sanchez et al. (2013)....
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...In Sanchez et al. (2013) we presented the first results based on the catalog of H ii regions extracted from these galaxies....
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...Similar results were found for the stellar masses (derived as described in Sanchez et al. 2013), and the C-index....
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304 citations
Cites background from "Mass-metallicity relation explored ..."
...However, the redshift independence of the relation between stellar mass, metallicity and SFR remains tentative (Niino 2012; Pérez-Montero et al. 2013; Sánchez et al. 2013; Zahid et al. 2013b; Ly et al. 2014)....
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269 citations
Cites background from "Mass-metallicity relation explored ..."
...The combination with the low-resolution V500 grating allows for mapping of stellar ages, metallicities, full star-formation histories, ionised-gas emission line fluxes, and chemical abundances (e.g. Pérez et al. 2013; Sánchez et al. 2013; Falcón-Barroso et al. in prep.)....
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257 citations
References
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"Mass-metallicity relation explored ..." refers methods in this paper
...The observed Hα intensities were corrected for reddening using the Balmer decrement (Hα/Hβ) according to the reddening function of Cardelli et al. (1989), assumingR≡ AV/E(B− V) = 3.1....
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10,039 citations
9,835 citations
"Mass-metallicity relation explored ..." refers methods in this paper
...So far, all the studies reporting a dependence between theMZ relation and the SFR are based on single aperture spectroscopic data, like the one provided by the SDSS survey (York et al. 2000)....
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"Mass-metallicity relation explored ..." refers background or methods in this paper
...This surface was already discussed by Rosales-Ortega et al. (2012), who, instead of using the sSFR used the equivalent width of Hα, a well-known proxy for the former parameter (e.g. Kennicutt 1998)....
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...The values of the SFR were derived for each galaxy adopting the classical relations by Kennicutt (1998), based on the dustcorrected Hα luminosities....
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...Based on the Schmidt-Kennicutt law, the surface SFR depends on the surface mass density,µSFR ∝ Σgasn (Kennicutt 1998), with a slope larger than one (n ∼ 1.4− 1.5)....
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...Its nature is still under debate (e.g. Davé 2008; Vulcani et al. 2010), but it is most probably related to the ability of a certain galaxy to acquire neutral gas, together with thewell known Schmidt-Kennicutt law (Kennicutt 1998)....
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