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Details

Autor(en) / Beteiligte
Titel
A low-mass cut-off near the hydrogen burning limit for Salpeter-like initial mass functions in early-type galaxies
Ist Teil von
  • Monthly notices of the Royal Astronomical Society, 2013-11, Vol.436 (1), p.253-258
Ort / Verlag
London: Oxford University Press
Erscheinungsjahr
2013
Link zum Volltext
Quelle
Alma/SFX Local Collection
Beschreibungen/Notizen
  • We conduct a detailed investigation of the properties of the stellar initial mass function (IMF) in two massive early-type lens galaxies with velocity dispersions of σ 245 and 325 km s−1, for which both Hubble Space Telescope imaging and X-Shooter spectra are available. We compare the inferences obtained from two fully independent methods: (i) a combined gravitational lensing and stellar dynamics (L&D) analysis of the data sets employing self-consistent axisymmetric models and (ii) a spectroscopic simple stellar population (SSP) analysis of optical line-strength indices, assuming single power-law IMFs. The results from the two approaches are found to be in agreement within the 1σ uncertainties. Both galaxies are consistent with having a Salpeter IMF (power-law slope of x = 2.35), which is strongly favoured over a Chabrier IMF (x = 1.8), with probabilities inferred from the joint analysis of 89 and 99 per cent, respectively. Bottom-heavy IMFs significantly steeper than Salpeter (x ≥ 3.0) are ruled out with decisive evidence (Bayes factor B > 1000) for both galaxies, as they exceed the total mass derived from the L&D constraints. Our analysis allows, for the first time, the inference of the low-mass cut-off of the IMF (M low). Combining the joint L&D and SSP analyses of both galaxies, we infer an IMF slope of x = 2.22 ± 0.14, consistent with Salpeter IMF and a low-mass limit M low = 0.13 ± 0.03  M, just above the hydrogen burning limit.
Sprache
Englisch
Identifikatoren
ISSN: 0035-8711
eISSN: 1365-2966
DOI: 10.1093/mnras/stt1727
Titel-ID: cdi_proquest_journals_1449478224

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