Intergalactic Magnetic Fields and the Morphology of Spiral Galaxies-Reference-Cited by-同舟云学术

Intergalactic Magnetic Fields and the Morphology of Spiral Galaxies

Published:1990 Issue: Volume:140 Page:504-506
ISSN:0074-1809
Container-title:Symposium - International Astronomical Union
language:en
Short-container-title:Symp. - Int. Astron. Union

Author:

Battaner E.,Florido E.,Sanchez-Saavedra M.L.

Abstract

The influence of the hypothetical extragalactic magnetic field upon the peripherical morphological features of spiral galaxies is examined- When the angle between and the rotation axis is neither 0° nor 90°, warps are expected to be produced. In such a case the spatial distribution of warps should not be random. This fact seems to be confirmed by observations. From the distribution it is possible to obtain the direction of B in the 20Mpc-neighborhood of the Milky Way.

Publisher

Cambridge University Press (CUP)

Reference7 articles.

1. ‘Surface photometry of the warping edge-on galaxy NGC 5907’;Sasaki;Publ. Astron. Soc. Japan,1987

2. Sanchez-Saavedra M.L. , Battaner E. and Florido E. (1989) ‘Statistical study of optical galactic warps’ in New windows in the Universe. Spinger Verlag, in press.

3. Battaner E. , Florido E. and Sanchez-Saavedra M.L. (1989b) ‘The role of magnetic fields in the evolution of galaxies’ in Beckman J.E. (ed.), Evolutionary Phenomena in Galaxies, Cambridge University Press, in press.

4. ‘The interpretation of rotation measures of extragalactic radio sources’;Ruzmaikin;Astron. Astrophys.,1977

5. Florido E. , Battaner E. and Sanchez-Saavedra M.L. (1989) ‘The Milky Way disk Warp’ in I.A.U. Symposium 120, Structure and dynamics of the interstellar medium, in press.

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