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Mass-to-Light Ratios of Globular Clusters in M31 (and the Milky Way)
HLA
Jay Strader
M31: 225-280
(with Nelson Caldwell, Anil Seth, Matt Walker, Mario Mateo)
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Mass-to-Light and [Fe/H]
12.5 Gyr
MP
MR
(in the optical)
normalizationmay vary
Kroupa IMF
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Mass-to-Light and [Fe/H]
MP
MR
(in the near-IR)
12.5 Gyr
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M31 GCs: Calculating M/L
high-res spectra + cluster structure
good imaging (pref HST)
![Page 5: Jay Strader - ESO · Mass-to-Light Ratios of Globular Clusters in M31 (and the Milky Way) HLA Jay Strader M31: 225-280 (with Nelson Caldwell, Anil Seth, Matt Walker, Mario Mateo)](https://reader034.vdocuments.site/reader034/viewer/2022042807/5f7a69f185d8bb1f6355ac5f/html5/thumbnails/5.jpg)
M/L of 27 M31 GCsStrader et al. 2009
Mostly multi-orderKeck/Lick spectra
[Fe/H]
log M/L
Djorgovski et al 1997
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M/L of 131 M31 GCsStrader et al. 2011
Mostly single-orderMMT spectra
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K-band M/LStrader et al. 2011
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M/L with Mass
Strader et al. 2011
Kruijssen models renormalized
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Ways to make M/L low
(i) Remove stars with high M/L(low-mass dwarfs)
(ii) Add stars with low M/L (RGB/AGB)
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Mass Function and M/L
(0.5 - 1 M )
typical GCs
most metal-rich GCs
KroupaIMF
Strader et al. 2011
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MF implicationsFor metal-rich M31 GCs, favors:
van Dokkum & Conroy (2010)
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Galactic GCs