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Les Regions Externes des Galaxies Ne Sont Pas Orientees Au Hasard

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Clusters and Groups of Galaxies

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 111))

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Résumé

Des halos (ou couronnes) peuvent être détectées autour d’un certain nombre de galaxies par:

  • la présence d’une enveloppe d’hydrogène neuter

  • la présence de galaxies naines satellites (cf. La Galaxie ou M 31) ou de galaxies compagnons (M 51).

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References

  • DE VAUCOULEURS, G.: 1975, Astron. Astrophys. 202, 319

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  • FLICHE, H.H., SOURIAU, J.M., TRIAY, R.: 1982, prétirage C.P.T.-83/P.1402, C.N.R.S., Marseille

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  • FLICHE, H.H., SOURIAU, J.M., TRIAY, R.: 1983, prétirage C.P.T.-83/P.1502, C.N.R.S., Marseille

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© 1984 D. Reidel Publishing Company

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Fliche, H.H., Souriau, J.M. (1984). Les Regions Externes des Galaxies Ne Sont Pas Orientees Au Hasard. In: Mardirossian, F., Giuricin, G., Mezzetti, M. (eds) Clusters and Groups of Galaxies. Astrophysics and Space Science Library, vol 111. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-6412-9_16

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  • DOI: https://doi.org/10.1007/978-94-009-6412-9_16

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-009-6414-3

  • Online ISBN: 978-94-009-6412-9

  • eBook Packages: Springer Book Archive

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