Skip to main content

Importance of Magellanic Clouds Studies for Extra-Galactic Work

  • Chapter
The Magellanic Clouds

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 23))

  • 73 Accesses

Abstract

The apparently early evolutionary state of the Magellanic Clouds, while they are coeval with the Galaxy in their earliest star condensations, may be due to perturbation by the Galaxy as well as to their low mass and low density. Whereas classical barred spirals are probably characterised by large angular momentum, the Clouds may owe their ‘barred’ and asymmetrical distribution, including departure of the centre of rotation from the geometrical centre, to local fluctuations in H1 density and rate of star formation at different epochs. Comparison is made with some other asymmetrical galaxies.

This is a preview of subscription content, log in via an institution to check access.

Access this chapter

Chapter
USD 29.95
Price excludes VAT (USA)
  • Available as PDF
  • Read on any device
  • Instant download
  • Own it forever
eBook
USD 84.99
Price excludes VAT (USA)
  • Available as PDF
  • Read on any device
  • Instant download
  • Own it forever
Softcover Book
USD 109.99
Price excludes VAT (USA)
  • Compact, lightweight edition
  • Dispatched in 3 to 5 business days
  • Free shipping worldwide - see info
Hardcover Book
USD 109.99
Price excludes VAT (USA)
  • Durable hardcover edition
  • Dispatched in 3 to 5 business days
  • Free shipping worldwide - see info

Tax calculation will be finalised at checkout

Purchases are for personal use only

Institutional subscriptions

Preview

Unable to display preview. Download preview PDF.

Unable to display preview. Download preview PDF.

References

  • Arp, H. C.: 1964, in F. J. Kerr and A. W. Rodgers (eds.), ‘The Galaxy and the Magellanic Clouds’, IAU-URSI Symp. 20, 219.

    Google Scholar 

  • Avner, E. S. and King, I. R.: 1967, Astron. J. 72, 650.

    Article  ADS  Google Scholar 

  • Bertola, F.: 1966, Contr. Obs. Astrophys. Asiago, Nos. 172, 186.

    Google Scholar 

  • Burbidge, E. M. and Burbidge, G. R.: 1966, Astrophys. J. 145, 661.

    Article  ADS  Google Scholar 

  • Burbidge, E. M., Burbidge, G. R., and Hoyle, F.: 1963, Astrophys. J. 138, 873.

    Article  ADS  Google Scholar 

  • Burbidge, E. M., Burbidge, G. R., and Prendergast, K. H.: 1960, Astrophys. J. 132, 654.

    Article  ADS  Google Scholar 

  • Holmberg, E.: 1964, Arkiv Astron. 3, 387.

    ADS  Google Scholar 

  • Prendergast, K. H. and Miller, R.: 1969, private communication.

    Google Scholar 

  • Schwarzschild, M.: 1954, Astron. J. 59 272.

    Article  Google Scholar 

  • Thackeray, A. D.: 1964, in F. J. Kerr and A. W. Rodgers (eds.), ‘The Galaxy and the Magellanic Clouds’, IAU-URSI Symp. 20, 380.

    Google Scholar 

  • Vaucouleurs, G. de: 1954, Observatory 74, 23.

    ADS  Google Scholar 

  • Vaucouleurs, G. de: 1955, Astron. J. 60, 126.

    Article  ADS  Google Scholar 

  • Vorontsov-Velyaminov, B. A.: 1959, Atlas of Interacting Galaxies Moscow.

    Google Scholar 

  • Walker, M. F. and Chincarini, G.: 1967, Astrophys. J. 147, 416.

    Article  ADS  Google Scholar 

Download references

Author information

Authors and Affiliations

Authors

Editor information

Editors and Affiliations

Rights and permissions

Reprints and permissions

Copyright information

© 1971 Springer Science+Business Media Dordrecht

About this chapter

Cite this chapter

Burbidge, E.M. (1971). Importance of Magellanic Clouds Studies for Extra-Galactic Work. In: Muller, A.B. (eds) The Magellanic Clouds. Astrophysics and Space Science Library, vol 23. Springer, Dordrecht. https://doi.org/10.1007/978-94-015-6906-4_21

Download citation

  • DOI: https://doi.org/10.1007/978-94-015-6906-4_21

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-015-6908-8

  • Online ISBN: 978-94-015-6906-4

  • eBook Packages: Springer Book Archive

Publish with us

Policies and ethics