articleThe Astronomical JournalNov 10, 2016BRONZE OA

SPARC: MASS MODELS FOR 175 DISK GALAXIES WITH SPITZER PHOTOMETRY AND ACCURATE ROTATION CURVES

FLFederico LelliSSStacy S. McGaughJMJames M. Schombert

Case Western Reserve University · University of Oregon

Indexed inarxivcrossrefdoaj

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…

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Authors

3
  • FL
    Federico LelliCorresponding

    Case Western Reserve University

  • SS
    Stacy S. McGaugh

    Case Western Reserve University

  • JM
    James M. Schombert

    University of Oregon

Topics & keywords

Keywords
  • Photometry (optics)
  • Galaxy rotation curve
  • Galaxy
  • Spiral galaxy
  • Stellar mass
  • Stellar population
  • Elliptical galaxy
  • Surface brightness fluctuation
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