Document Type

Article

Publication Date

7-2013

Department

Physics and Astronomy

Abstract

We have analyzed the radial distribution of old stars in a sample of 218 nearby face-on disks, using deep 3.6μm images from the Spitzer Survey of Stellar Structure in Galaxies. In particular, we have studied the structural properties of those disks with a broken or down-bending profile. We find that, on average, disks with a genuine single-exponential profile have a scale length and a central surface brightness which are intermediate to those of the inner and outer components of a down-bending disk with the same total stellar mass. In the particular case of barred galaxies, the ratio between the break and the bar radii (Rbr/Rbar) depends strongly on the total stellar mass of the galaxy. For galaxies more massive than 1010 M, the distribution is bimodal, peaking at Rbr/Rbar ∼ 2 and ∼3.5. The first peak, which is the most populated one, is linked to the outer Lindblad resonance of the bar, whereas the second one is consistent with a dynamical coupling between the bar and the spiral pattern. For galaxies below 1010 M, breaks are found up to ∼10 Rbar, but we show that they could still be caused by resonances given the rising nature of rotation curves in these low-mass disks. While not ruling out star formation thresholds, our results imply that radial stellar migration induced by non-axisymmetric features can be responsible not only for those breaks at ∼2 Rbar, but also for many of those found at larger radii.

Comments

Copyright 2013. The American Astronomical Society. All rights reserved.

https://doi.org/10.1088/0004-637X/771/1/59

Original Publication Information

Munoz-Mateos, Juan Carlos, et al. "The Impact of Bars on Disk Breaks as Probed by S4G Imaging." 2013. The Astrophysical Journal 771(1): 30 pp.

DOI

10.1088/0004-637X/771/1/59

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