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Sparc: Mass Models for 175 Disk Galaxies With Spitzer Photometry and Accurate Rotation Curves

Year: 2016
Type: article
Abstract: ABSTRACT We introduce SPARC ( Spitzer Photometry and Accurate Rotation Curves): a sample of 175 nearby galaxies with new surface photometry at 3.6 μ m and high-quality rotation curves from previous H i /H α studies. SPARC spans a broad range of morphologies (S0 to Irr), luminosities (∼5 dex), and surface brightnesses (∼4 dex). We derive [3.6] surface photometry and study structural relations of stellar and gas disks. We find that both the stellar mass–H i mass relation and the stellar radius–H i radius relation have significant intrinsic scatter, while the H i mass–radius relation is extremely tight. We build detailed mass models and quantify the ratio of baryonic to observed velocity ( V bar / V obs ) for different characteristic radii and values of the stellar mass-to-light ratio (ϒ ⋆ ) at [3.6]. Assuming ϒ ⋆ ≃ 0.5 M ⊙ / L ⊙ (as suggested by stellar population models), we find that (i) the gas fraction linearly correlates with total luminosity; (ii) the transition from star-dominated to gas-dominated galaxies roughly corresponds to the transition from spiral galaxies to dwarf irregulars, in line with density wave theory; and (iii) V bar / V obs varies with luminosity and surface brightness: high-mass, high-surface-brightness galaxies are nearly maximal, while low-mass, low-surface-brightness galaxies are submaximal. These basic properties are lost for low values of ϒ ⋆ ≃ 0.2 M ⊙ / L ⊙ as suggested by the DiskMass survey. The mean maximum-disk limit in bright galaxies is ϒ ⋆ ≃ 0.7 M ⊙ / L ⊙ at [3.6]. The SPARC data are publicly available and represent an ideal test bed for models of galaxy formation.
DOI: 10.3847/0004-6256/152/6/157
Authors: Federico Lelli, Stacy S. McGaugh, James M. Schombert
Language: English
Open Access status: bronze
OpenAlex ID: W2464805820
FWCI: 20.91
Cites: 123
Cited by: 956
Related to: 10