SPARC: MASS MODELS FOR 175 DISK GALAXIES WITH SPITZER PHOTOMETRY AND ACCURATE ROTATION CURVES
Case Western Reserve University · University of Oregon
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…
Citation impact
- FWCI
- 28.19
- Percentile
- 100%
- References
- 107
Authors
3- FLFederico LelliCorresponding
Case Western Reserve University
- SSStacy S. McGaugh
Case Western Reserve University
- JMJames M. Schombert
University of Oregon
Topics & keywords
- Photometry (optics)
- Galaxy rotation curve
- Galaxy
- Spiral galaxy
- Stellar mass
- Stellar population
- Elliptical galaxy
- Surface brightness fluctuation