The DiskMass Survey VII. The distribution of luminous and dark matter in spiral galaxies
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...The black pentagons show observational results for spiral galaxies at redshift z ≃ 0 from the DiskMass project (Bershady et al. 2010; Martinsson et al. 2013)....
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...• The observed concentrations and halo masses from NFW fits to data of spiral galaxies from the DiskMass project (Bershady et al. 2010; Martinsson et al. 2013), groups and clusters of galaxies (Ettori et al. 2010; Auger et al. 2013) are in good agreement with our simulations suggesting only mild…...
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References
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"The DiskMass Survey VII. The distri..." refers methods in this paper
...…gas kinematics from SparsePak (Bershady et al. 2004, 2005), as well as 21-cm radio synthesis data from the WSRT, GMRT and VLA, nearinfrared (NIR) photometry from the Two-Micron All-Sky Survey (2MASS; Skrutskie et al. 2006) and MIPS 24-µm imaging from the Spitzer Space Telescope (hereafterSpitzer)....
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...Fromnumerical N-body simulations (e.g., Navarro et al. 1997) the inner density profiles and concentrations of the dark-matter halos re predicted in the absence of baryons....
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...(6) The NFW halo is parameterized by its mass (Mhalo200) within the virial radius (R200; defined as the radius of a sphere of mean interior density 200 times the critical densityρcrit=3H20/8πG) and its concentration (C) as defined in Navarro et al. (1997)....
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...…into Cases Ia and IIa, which have a parameterized dark-matter halo modeled as a spherical pseudo-isothermal sphere (pISO; e.g., Ostriker & Caldwe l 1979; Schmidt 1985; Kent 1986), and Cases Ib and IIb which instead include a Navarro-Frenk-White (NFW; Navarro et al. 1997) dark-matter-halo model....
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"The DiskMass Survey VII. The distri..." refers methods in this paper
...Distances are taken from Paper I. Integrated Hi fluxes ( ∫ S HIdV) are from tabulated values in NED, with three different sources; 1(RC3; de Vaucouleurs et al. 1991),2(HIPASS; Doyle et al. 2005), 3(Andersen et al. 2006)....
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3,094 citations
"The DiskMass Survey VII. The distri..." refers background in this paper
...…mass-to-light ratio of the stellar component (Υ∗) until the rotation curve of the baryons approximates the amplitude of the erations (e.g., Milgrom 1983; Begeman et al. 1991; Sanders 1996; Sanders & Verheijen 1998). observed rotation curve in the inner region (the “maximum-disk…...
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