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Early-type Galaxies with Tidal Debris and Their Scaling Relations in the Spitzer Survey of Stellar Structure in Galaxies (S4G)




TekijätKim T, Sheth K, Hinz J, Lee M, Zaritsky D, Gadotti D, Knapen J, Schinnerer E, Ho L, Laurikainen E, Salo H, Athanassoula E, Bosma A, de Swardt B, Munoz-Mateos J-C, Madore B, Comeron S, Regan M, Mendez-Delmestre K, Gil de Paz A, Seibert M, Laine J

KustantajaInstitute of Physics (IOP)

KustannuspaikkaMcMaster University, 1280 Main Street West, GSB-118C, Hamilton, ON L8S 4K1

Julkaisuvuosi2012

JournalAstrophysical Journal

Lehden akronyymiApJ

Vuosikerta753

Numero1

Aloitussivu43

Lopetussivu60

Sivujen määrä18

ISSN0004-637x

eISSN0004-637x

DOIhttps://doi.org/10.1088/0004-637X/753/1/43


Tiivistelmä
Tidal debris around galaxies can yield important clues on their evolution. We have identified tidal debris in 11 early-type galaxies (T <= 0) from a sample of 65 early types drawn from the Spitzer Survey of Stellar Structure in Galaxies (S4G). The tidal debris includes features such as shells, ripples, and tidal tails. A variety of techniques, including two-dimensional decomposition of galactic structures, were used to quantify the residual tidal features. The tidal debris contributes ~3%-10% to the total 3.6 μm luminosity of the host galaxy. Structural parameters of the galaxies were estimated using two-dimensional profile fitting. We investigate the locations of galaxies with tidal debris in the fundamental plane and Kormendy relation. We find that galaxies with tidal debris lie within the scatter of early-type galaxies without tidal features. Assuming that the tidal debris is indicative of recent gravitational interaction or merger, this suggests that these galaxies have either undergone minor merging events so that the overall structural properties of the galaxies are not significantly altered, or they have undergone a major merging events but already have experienced sufficient relaxation and phase mixing so that their structural properties become similar to those of the non-interacting early-type galaxies.



Last updated on 2024-26-11 at 19:40