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Magnetic Fields and the Interstellar Medium in Spiral Arms

Published online by Cambridge University Press:  25 May 2016

M. Urbanik ,
M. Soida  and
R. Beck
M. Urbanik
Affiliation:
Astronomical Observatory, Jagiellonian University, ul. Orla 171, Krakow, Poland
M. Soida
Affiliation:
Astronomical Observatory, Jagiellonian University, ul. Orla 171, Krakow, Poland
R. Beck
Affiliation:
Max-Planck Institut für Radiastronomie Auf dem Hügel 69, Bonn, Germany

Extract

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We performed the high frequency radio studies of spiral galaxies using the 100 m MPIfR radio telescope at 10.55 GHz. Two objects: NGC 4254 and NGC 3627 possess perturbed spiral structures while two others, NGC 3521 and NGC 5055 are flocculent objects, lacking organized spiral patterns. NGC 3521 possesses also a peculiar dust lane. For NGC 4254, NGC 3627 and NGC 5055 deep polarization maps were made, for NGC 3521 the total power data only were analyzed (see Urbanik et al. 1989).

Type
Poster Papers
Information
Symposium - International Astronomical Union , Volume 171: New Light on Galaxy Evolution , 1996 , pp. 456
Copyright
Copyright © Kluwer 1996 

References

Elstner, D., Meinel, R., Beck, R.: 1992, Astron. Astrophys. Suppl. 94, 587 Google Scholar
Soida, M., Urbanik, M. Beck, R.: 1995, Astron. Astrophys. submitted Google Scholar
Urbanik, M., Beck, R., Klein, U., Gräve, R.: 1989 Astrophys. Space. Sci. 156, 195 Google Scholar