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Symposium - International Astronomical Union
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Symposium - International Astronomical Union
Article . 1983 . Peer-reviewed
License: Cambridge Core User Agreement
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https://doi.org/10.1007/978-94...
Part of book or chapter of book . 1983 . Peer-reviewed
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https://dx.doi.org/10.1007/978...
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The Origin Of Dwarf Spheroidal Galaxies

descriptionPublicationkeyboard_double_arrow_right Part of book or chapter of book , Article , Other literature type 01 Jan 1983 English Publisher:Springer NetherlandsJournal:Symposium - International Astronomical Union, volume 100, pages 89-92 (issn: 0074-1809, Copyright policy )
Authors: D. Lynden-Bell;

doi: 10.1007/978-94-009-7075-5_21 , 10.1017/s0074180900032484

The Origin Of Dwarf Spheroidal Galaxies

Abstract

Two dwarf spheroidal galaxies are associated with the Magellanic Stream with their major axes oriented along it. Evidence suggests that all the dwarf spheroidal satellites of the Galaxy belong to one or other of two streams of tidal debris. If this is true the orbits will give the first reliable determination of the total mass of the Galaxy out to 120 kpc.

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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
17
Average
Average
Average
bronze
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