papers

Publications (12)

astro-ph.GA2018

Nonaxisymmetric models of galaxy velocity maps

Francesco Sylos Labini, David Benhaiem, Sebastien Comeron +1

Galaxy velocity maps often show the typical pattern of a rotating disk, consistent with the dynamical model where emitters rotate in circular orbits around the galactic center. The…

astro-ph.GA2014

IRAC Near-Infrared Features in the Outer Parts of S4G Galaxies

Seppo Laine, Johan H. Knapen, Juan-Carlos Munoz-Mateos +26

We present a catalogue and images of visually detected features, such as asymmetries, extensions, warps, shells, tidal tails, polar rings, and obvious signs of mergers or interacti…

astro-ph.GA2013

Embedded Star Formation in S4G Galaxy Dust Lanes

Debra M. Elmegreen, Bruce G. Elmegreen, Santiago Erroz-Ferrer +22

Star-forming regions that are visible at 3.6 microns and Halpha but not in the u,g,r,i,z bands of the Sloan Digital Sky survey (SDSS), are measured in five nearby spiral galaxies t…

astro-ph.CO2012

The S4G perspective on circumstellar dust extinction of AGB stars in M100

Sharon E. Meidt, Eva Schinnerer, Juan-Carlos Munoz-Mateos +19

We examine the effect of circumstellar dust extinction on the near-IR contribution of asymptotic giant branch (AGB) stars in intermediate-age clusters throughout the disk of M100.…

astro-ph.GA2016

Halpha Kinematics of S4G Spiral Galaxies - III. Inner rotation curves

Santiago Erroz-Ferrer, Johan H. Knapen, Ryan Leaman +10

We present a detailed study of the shape of the innermost part of the rotation curves of a sample of 29 nearby spiral galaxies, based on high angular and spectral resolution kinema…

astro-ph.GA2015

A Classical Morphological Analysis of Galaxies in the Spitzer Survey of Stellar Structure in Galaxies (S4G)

R. Buta, K. Sheth, E. Athanassoula +22

The Spitzer Survey of Stellar Structure in Galaxies (S4G) is the largest available database of deep, homogeneous middle-infrared (mid-IR) images of galaxies of all types. The surve…

astro-ph.GA2015

The Spitzer Survey of Stellar Structure in Galaxies (S4G): Stellar Masses, Sizes and Radial Profiles for 2352 Nearby Galaxies

Juan Carlos Munoz-Mateos, Kartik Sheth, Michael Regan +25

The Spitzer Survey of Stellar Structure in Galaxies (S4G) is a volume, magnitude, and size-limited survey of 2352 nearby galaxies with deep imaging at 3.6 and 4.5um. In this paper…

astro-ph.GA2023

The truncation of the disk of NGC 4565: Detected up to z=4 kpc, with star formation, and affected by the warp

Cristina Martinez-Lombilla, Raul Infante-Sainz, Felipe Jimenez-Ibarra +5

Context: The hierarchical model of galaxy formation suggests that galaxies are continuously growing. However, our position inside the Milky Way prevents us from studying the disk e…

astro-ph.GA2024

Gas flows in the central region of the Seyfert galaxy NGC 4593 with MUSE

Dorcus Mulumba, Johan Knapen, Sebastien Comeron +4

Understanding how gas flows into galactic centres, fuels the AGN, and is in turn expelled back through feedback processes is of great importance to appreciate the role AGN play in…

astro-ph.CO2009

On the curvature of dustlanes in galactic bars

Sebastien Comeron, Inma Martinez-Valpuesta, Johan H. Knapen +1

We test the theoretical prediction that the straightest dust lanes in bars are found in strongly barred galaxies, or more specifically, that the degree of curvature of the dust lan…

astro-ph.CO2011

Reconstructing the stellar mass distributions of galaxies using S4G IRAC 3.6 and 4.5 micron images: I. Correcting for contamination by PAH, hot dust, and intermediate age stars

Sharon E. Meidt, Eva Schinnerer, Johan H. Knapen +23

With the aim of constructing accurate 2D maps of the stellar mass distribution in nearby galaxies from S4G 3.6 and 4.5 micron images, we report on the separation of the light from…

astro-ph.GA2014

Reconstructing the stellar mass distributions of galaxies using S4G IRAC 3.6 and 4.5 micron images: II. The conversion from light to mass

Sharon E. Meidt, Eva Schinnerer, Glenn van de Ven +26

We present a new approach for estimating the 3.6 micron stellar mass-to-light ratio in terms of the [3.6]-[4.5] colors of old stellar populations. Our approach avoids several of th…