Home News About Us Contact Contributors Disclaimer Privacy Policy Help FAQ

Home
Search
Quick Search
Advanced
Fulltext
Browse
Collections
Persons
My eDoc
Session History
Login
Name:
Password:
Documentation
Help
Support Wiki
Direct access to
document ID:


          Institute: MPI für Astronomie     Collection: Publikationen_mpia     Display Documents



ID: 693826.0, MPI für Astronomie / Publikationen_mpia
X-ray nuclear activity in S4G barred galaxies: no link between bar strength and co-occurrent supermassive black hole fueling
Authors:Cisternas, M.; Gadotti, D. A.; Knapen, J. H.; Kim, T.; Díaz-García, S.; Laurikainen, E.; Salo, H.; González-Martín, O.; Ho, L. C.; Elmegreen, B. G.; Zaritsky, D.; Sheth, K.; Athanassoula, E.; Bosma, A.; Comerón, S.; Erroz-Ferrer, S.; Gil de Paz, A.; Hinz, J. L.; Holwerda, B. W.; Laine, J.; Meidt, S.; Menéndez-Delmestre, K.; Mizusawa, T.; Muñoz-Mateos, J. C.; Regan, M. W.; Seibert, M.
Date of Publication (YYYY-MM-DD):2013
Title of Journal:The Astrophysical Journal
Volume:776
Issue / Number:1
Start Page:id. 50 (15 pp)
Audience:Not Specified
Abstract / Description:Stellar bars can lead to gas inflow toward the center of a galaxy and stimulate nuclear star formation. However, there is no compelling evidence on whether they also feed a central supermassive black hole: by measuring the fractions of barred active and inactive galaxies, previous studies have yielded conflicting results. In this paper, we aim to understand the lack of observational evidence for bar-driven active galactic nucleus (AGN) activity by studying a sample of 41 nearby (d < 35 Mpc) barred galaxies from the Spitzer Survey for Stellar Structure in Galaxies. We use Chandra observations to measure nuclear 2-10 keV X-ray luminosities and estimate Eddington ratios, together with Spitzer 3.6 μm imaging to quantify the strength of the stellar bar in two independent ways: (1) from its structure, as traced by its ellipticity and boxiness, and (2) from its gravitational torque Qb , taken as the maximum ratio of the tangential force to the mean background radial force. In this way, rather than discretizing the presence of both stellar bars and nuclear activity, we are able to account for the continuum of bar strengths and degrees of AGN activity. We find nuclear X-ray sources in 31 out of 41 galaxies with median X-ray luminosity and Eddington ratio of L X = 4.3 × 1038 erg s-1 and L bol/L Edd = 6.9 × 10-6, respectively, consistent with low-luminosity AGN activity. Including upper limits for those galaxies without nuclear detections, we find no significant correlation between any of the bar strength indicators and the degree of nuclear activity, irrespective of galaxy luminosity, stellar mass, Hubble type, or bulge size. Strong bars do not favor brighter or more efficient nuclear activity, implying that at least for the low-luminosity regime, supermassive black hole fueling is not closely connected to large-scale features.
Free Keywords:galaxies: active; galaxies: evolution; galaxies: nuclei; galaxies: structure
External Publication Status:published
Document Type:Article
Communicated by:N. N.
Affiliations:MPI für Astronomie
Identifiers:ISSN:0004-637X %R 10.1088/0004-637X/776/1/50
URL:http://cdsads.u-strasbg.fr/abs/2013ApJ...776...50C
The scope and number of records on eDoc is subject to the collection policies defined by each institute - see "info" button in the collection browse view.