Star formation timescales in M82

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5 Citations (Scopus)

Abstract

The last tidal encounter between M82 and M81, some 500 Myr ago, had a major impact on what was probably an otherwise normal, quiescent disk galaxy. It caused a concentrated burst of star formation in the form of masive star clusters that decreased rapidly, within a few 100 Myr. The current starburst in the centre of the galaxy is likely to arise from large-scale propagating star formation. Alternatively, it may be related to late infall of tidally disrupted debris from M82 itself. Star formation here overall may, in fact, come from a combination of these two mechanisms, in the sense that the star formation in the active core is actively propagating, whilst the overall evolution of the starburst depends on tidal debris raining back onto the disk of the galaxy, giving rise to the present-day starburst.

Original languageEnglish
Pages (from-to)412-417
Number of pages6
JournalAstronomy and Geophysics
Volume42
Issue number4
DOIs
Publication statusPublished - Aug 2001
Externally publishedYes

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