Radio spectral index images of the spiral galaxies NGC 0628, NGC 3627, and NGC 7331

Astronomy and Astrophysics – Astrophysics – Cosmology and Extragalactic Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

12 pages, 11 figures, Accepted for pubblication in Astronomy & Astrophysics A high resolution version of the paper can be down

Scientific paper

In order to understand the cosmic ray propagation mechanism in galaxies, and its correlation with the sites of star formation, we compare the spatially resolved radio spectral index of three spiral galaxies with their IR distribution. We present new low-frequency radio continuum observations of the galaxies NGC 0628, NGC 3627, and NGC 7331, taken at 327 MHz with the Very Large Array. We complemented our data set with sensitive archival observations at 1.4 GHz and we studied the variations of the radio spectral index within the disks of these spiral galaxies. We also compared the spectral index distribution and the IR distribution, using 70 $\mu$m Spitzer observations. We found that in these galaxies the non-thermal spectral index is anticorrelated with the radio brightness. Bright regions, like the bar in NGC 3627 or the circumnuclear region in NGC 7331, are characterized by a flatter spectrum with respect to the underlying disk. Therefore, a systematic steepening of the spectral index with the increasing distance from the center of these galaxies is observed. Furthermore, by comparing the radio images with the 70 $\mu$m images of the Spitzer satellite we found that a similar anticorrelation exists between the radio spectral index and the infrared brightness, as expected on the basis of the local correlation between the radio continuum and the infrared emission. Our results support the idea that in regions of intense star formation the electron diffusion must be efficient. The observed anticorrelation between radio brightness and spectral index, may imply that the cosmic ray density and the magnetic field strength are significantly higher in these regions than in their surroundings.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Radio spectral index images of the spiral galaxies NGC 0628, NGC 3627, and NGC 7331 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Radio spectral index images of the spiral galaxies NGC 0628, NGC 3627, and NGC 7331, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Radio spectral index images of the spiral galaxies NGC 0628, NGC 3627, and NGC 7331 will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-325355

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.