J/A+A/568/A74        Low-frequency (115-175MHz) image of M51    (Mulcahy+, 2014)

The nature of the low-frequency emission of M51. First observations of a nearby galaxy with LOFAR. Mulcahy D.D., Horneffer A., Beck R., Heald G., Fletcher A., Scaife A., Adebahr B., Anderson J.M., Bonafede A., Brueggen M., Brunetti G., Chyzy K.T., Conway J., Dettmar R.-J., Ensslin T., Haverkorn M., Horellou C., Iacobelli M., Israel F.P., Junklewitz H., Jurusik W., Koehler J., Kuniyoshi M., Orru E., Paladino R., Pizzo R., Reich W., Roettgering H.J.A. <Astron. Astrophys. 568, A74 (2014)> =2014A&A...568A..74M 2014A&A...568A..74M
ADC_Keywords: Galaxies, nearby ; Radio continuum ; Polarization Keywords: polarization - ISM: cosmic rays - galaxies: individual: M51 - galaxies: ISM - galaxies: magnetic fields - radio continuum: galaxies Abstract: The grand-design spiral galaxy M51 was observed with the LOFAR High Frequency Antennas (HBA) and imaged in total intensity and polarization. This observation covered the frequencies between 115MHz and 175MHz. We produced an image of total emission of M51 at the mean frequency of 151MHz with 20-arcsec resolution and 0.3mJy rms noise, which is the most sensitive image of a galaxy at frequencies below 300MHz so far. The integrated spectrum of total radio emission is well described by a power law, while flat spectral indices in the central region indicates thermal absorption. We observe the disk to extend out to 16kpc and a break in the radial profile near the optical radius of the disk. The radial scale lengths in the inner and outer disks are larger at 151MHz, and the break is smoother at 151MHz than those observed at 1.4GHz. The arm--interarm contrast is lower at 151MHz than at 1400MHz, indicating propagation of cosmic ray electrons (CRE) from spiral arms into interarm regions. Description: Stokes I FITS image of M51 observed with LOFAR High Frequency Antennas (HBA) with a mean frequency of 151MHz at 20-arcsec resolution. Full details of the data reduction are explained in section 2 of the paper. Objects: -------------------------------------------- RA (2000) DE Designation(s) -------------------------------------------- 13 29 52.70 +47 11 42.9 M51 = NGC 5194 -------------------------------------------- File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file list.dat 71 1 List of image M51LOFARHBA.fits 2880 128 FITS image -------------------------------------------------------------------------------- Byte-by-byte Description of file: list.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 9 F9.5 deg RAdeg Right Ascension of center (J2000) 10- 18 F9.5 deg DEdeg Declination of center (J2000) 20 I1 arcsec/pix Scale [5] Scale of the image 22- 24 I3 --- Nx [301] Number of pixels along X-axis 25 A1 --- --- [x] 26- 28 I3 --- Ny [301] Number of pixels along Y-axis 30- 32 I3 Kibyte size [363] Size of the FITS image 34- 49 A16 --- FileName Name of the FITS image 51- 71 A21 --- Title Title of the file -------------------------------------------------------------------------------- Acknowledgements: David Mulcahy, D.D.Mulcahy(at)soton.ac.uk
(End) Patricia Vannier [CDS] 04-Jul-2014
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