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Cold dust in a selected sample of nearby galaxies. I. The interacting galaxy NGC4631 | | M. Dumke
; M. Krause
; R. Wielebinski
; | | Date: |
26 Nov 2003 | | Journal: | Astron.Astrophys. 414 (2004) 475-486 | | Subject: | astro-ph | | Affiliation: | 1 and 2), M. Krause , R. Wielebinski ( MPI fuer Radioastronomie, Bonn, SMTO, University of Arizona, Tucson, AZ | | Abstract: | We have observed the continuum emission of the interacting galaxy NGC4631 at 0.87 and 1.23mm using the Heinrich-Hertz-Telescope on Mt. Graham and the IRAM 30-m telescope on Pico Veleta. We have obtained fully sampled maps which cover the optical emission out to a radius of about 7’ at both wavelengths. For a detailed analysis, we carefully subtracted the line contributions and synchrotron and free-free emission from the data, which added up to 6% at 1.23mm and 10% at 0.87mm. We combined the flux densities with FIR data to obtain dust spectra and calculate dust temperatures, absorption cross sections, and masses. Assuming a ``standard’’ dust model, which consists of two populations of big grains at moderate and warm temperatures, we obtained temperatures of 18K and 50K for the both components. However, such a model suffers from an excess of the radiation at 1.23mm, and the dust absorption cross section seems to be enhanced by a factor 3 compared to previous results and theoretical expectations. At large galactocentric radii, where the galaxy shows disturbances as a result of gravitational interaction, this effect seems to be even stronger. Some possibilities to resolve these problems are discussed. The data could be explained by a very cold dust component at a temperature of 4-6K, an increased abundance of very small grains, or a component of grains with unusual optical properties. We favour the latter possibility, since the first two lead to inconsistencies. | | Source: | arXiv, astro-ph/0311591 | | Services: | Forum | Review | PDF | Favorites | |
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