Document Type

Article

Publication Date

11-11-2016

Abstract

We introduce SPARC (Spitzer Photometry and Accurate Rotation Curves): a sample of 175 nearby galaxies with new surface photometry at 3.6 μm and high-quality rotation curves from previous H I/Hα 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 (Vbar/Vobs) 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) Vbar/Vobs 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.

Keywords

dark matter, galaxies: dwarf, galaxies: irregular, galaxies: kinematics and dynamics, galaxies: spiral, galaxies: structure

Publication Title

Astronomical Journal

Rights

© The American Astronomical Society. All rights reserved. This content is free to access, download, and share. For all other uses, you must obtain permission to reuse content: https://journals.aas.org/article-charges-and-copyright/#AAS_material

Share

COinS
 

Manuscript Version

Final Publisher Version

 

To view the content in your browser, please download Adobe Reader or, alternately,
you may Download the file to your hard drive.

NOTE: The latest versions of Adobe Reader do not support viewing PDF files within Firefox on Mac OS and if you are using a modern (Intel) Mac, there is no official plugin for viewing PDF files within the browser window.