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: 709864.0, MPI für Astronomie / Publikationen_mpia
Dissecting the origin of the submillimetre emission in nearby galaxies with Herschel and LABOCA
Authors:Galametz, M.; Albrecht, M.; Kennicutt, R.; Aniano, G.; Bertoldi, F.; Calzetti, D.; Croxall, K. V.; Dale, D.; Draine, B.; Engelbracht, C.; Gordon, K.; Hinz, J.; Hunt, L. K.; Kirkpatrick, A.; Murphy, E.; Roussel, H.; Skibba, R. A.; Walter, F.; Weiss, A.; Wilson, C. D.
Date of Publication (YYYY-MM-DD):2014
Title of Journal:Monthly Notices of the Royal Astronomical Society
Volume:439
Issue / Number:3
Start Page:2542
End Page:2570
Audience:Not Specified
Abstract / Description:We model the infrared to submillimetre spectral energy distribution of 11 nearby galaxies of the Key Insights on Nearby Galaxies: A Far-Infrared Survey with Herschel sample using Spitzer and Herschel data and compare model extrapolations at 870 mum (using different fitting techniques) with Large APEX BOlometer CAmera (LABOCA) 870 mum observations. We investigate how the differences between predictions and observations vary with model assumptions or environment. At global scales, we find that modified blackbody models using realistic cold emissivity indices (betac = 2 or 1.5) are able to reproduce the 870 mum observed emission within the uncertainties for most of the sample. Low values (betac < 1.3) would be required in NGC 0337, NGC 1512 and NGC 7793. At local scales, we observe a systematic 870 mum excess when using betac = 2.0. The betac = 1.5 or the Draine & Li (2007) models can reconcile predictions with observations in part of the discs. Some of the remaining `excesses' occur towards the centres and can be partly or fully accounted for by non-dust contributions such as CO(3-2) or, to a lesser extent, free-free or synchrotron emission. In three non-barred galaxies, the remaining excesses rather occur in the disc outskirts. This could be a sign of a flattening of the submm slope (and decrease of the effective emissivity index) with radius in these objects.
Free Keywords:galaxies: ISM
External Publication Status:published
Document Type:Article
Communicated by:N. N.
Affiliations:MPI für Astronomie
Identifiers:ISSN:0035-8711 %R 10.1093/mnras/stu113
URL:http://cdsads.u-strasbg.fr/abs/2014MNRAS.439.2542G
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.