No CrossRef data available.
Article contents
A comparison of the Andromeda and Milky Way galaxies
Published online by Cambridge University Press: 04 August 2017
Abstract
Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.
A comparison of some of the basic properties of M31 and the Milky Way indicates that in almost every respect M31 is larger than the Galaxy. It is more luminous, redder, more massive, and of earlier Hubble type. A detailed comparison of the spiral structure, based on optical tracers, for comparable areas in the outer parts of each galaxy shows differences in the arm spacings, in density enhancement, and in pitch angle.
- Type
- PART II: COMPOSITION, STRUCTURE AND KINEMATICS
- Information
- Symposium - International Astronomical Union , Volume 106: The Milky Way Galaxy , 1985 , pp. 423 - 430
- Copyright
- Copyright © Reidel 1985
References
Deharveng, J.M., Jakobsen, P., Milliard, B., and Laget, M.: 1980, Astron Astrophys.
88, 52
Google Scholar
Kalnajs, A.: 1975, “La Dynamique des Galaxies Spirales”, ed. Weliachew, L., Paris, CNRS
No. 241
Google Scholar
Sargent, W.L.W., Kowal, C., Hartwick, D., and van den Bergh, S.: 1977, Astron. J.
82, 947
CrossRefGoogle Scholar
Simien, F., Athanassoula, E., Pellet, A., Monnet, G., Maucherat, A., and Courtès, G.: 1978, Astron. Astrophys.
67, 73
Google Scholar
van Speybroeck, L., Epstein, A., Forman, W., Giacconi, R., Jones, C., Liller, W., and Smarr, L.: 1979, Astrophys. J.
234, L49
Google Scholar
You have
Access