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Tidally-induced Super Star Clusters in M82

Tidally-induced Super Star Clusters in M82
Tidally-induced Super Star Clusters in M82

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Extragalactic Star Clusters IAU Symposium Series,Vol.Vol.207,2001Eva K.Grebel,Doug Geisler,and Dante Minniti,eds.Tidally-induced Super Star Clusters in M82R.de Grijs Institute of Astronomy,Univ.of Cambridge,Madingley Road,Cambridge CB30HA,UK R.W.O’Connell Astronomy Dept.,Univ.of Virginia,P.O.Box 3818,Charlottesville,VA 22903,USA J.S.Gallagher,iii Astronomy Dept.,Univ.of Wisconsin,475N.Charter Str.,Madison,WI 53706,USA https://www.doczj.com/doc/9718965171.html,ing new HST imaging,we identify a large,evolved system of super star clusters in a disk region just outside the starburst core in the prototypical starburst galaxy M82,“M82B.”This region has been suspected to be a fossil starburst site in which an intense episode of star formation occurred over 100Myr ago,which is now con?rmed by our derived age distribution.It suggests steady,continuing cluster formation at a modest rate at early times (>2Gyr ago),followed by a concentrated formation episode ~600Myr ago and more recent suppression of clus-ter formation.The peak episode coincides with independent dynamical estimates for the last tidal encounter with M81.1.M82,the prototypical starburst galaxy Observations from radio to X-rays show evidence for a tidally-induced starburst

in the center of M82(e.g.,Telesco 1988)In fact,there is now evidence that M82has undergone multiple episodes of intense star formation (cf.Marcum &O’Connell 1996,de Grijs,O’Connell &Gallagher 2001).“M82B,”the fossil starburst region,has exactly the properties of an evolved starburst with a similar amplitude to the active burst (Marcum &O’Connell 1996).Thus,M82is a unique starburst galaxy,since no other galaxy o?ers the opportunity to study two discrete starbursts at such close range!By analogy with the HST results from the active starburst region (O’Connell et al.1994,1995),we expected M82B to have contained a complement of luminous super star clusters.It is possible that most of the star formation in starbursts takes place in the form of such concentrated clusters;in M82,we do not observe any outside the starburst regions.

The combination of observations of both the active and the fossil starburst sites in M82provides a unique physical environment for the study of the stellar and dynamical evolution of star cluster systems

1

2R.de Grijs et al.

Figure1.Age distribution of the star clusters in M82B.Shaded his-

togram:well-determined ages;open histogram:upper or lower limits

only(cf.de Grijs et al.2001).

2.The star formation history in M82

Based on HST/WFPC2observations of two adjacent?elds in M82B(in F439W, F555W and F814W),we detected~100(slightly)evolved star clusters.The clusters brighter than V=22.5exhibit a wide range of ages,from~30Myr to over10Gyr.There is a strong peak of cluster formation at~600Myr,in either representation in Fig.1;very few clusters are younger than300Myr.

Our results suggest steady,continuing cluster formation at a very modest rate at early times(>2Gyr ago),followed by a concentrated formation episode lasting from400–1000Myr ago and a subsequent suppression of cluster forma-tion.Thus,it appears that the last tidal encounter between M82and M81~500–800Myr ago had a major impact on what was probably an otherwise nor-mal,quiescent,disk galaxy.It caused a concentrated burst of star formation activity,which decreased rapidly within a few hundred Myr.

M82B has evidently not been a?ected by the more recent(<30Myr) starburst episode now continuing in the central regions.

References

de Grijs R.,O’Connell R.W.,Gallagher J.S.,2001,AJ,121,768

Marcum P.,O’Connell R.W.1996,in:From Stars to Galaxies:The Impact of Stellar Physics on Galaxy Evolution,eds.Leitherer C.,Fritze-von Alvensleben U.,Huchra J.,San Francisco:ASP,p.419

O’Connell R.W.,Gallagher J.S.,Hunter D.A.1994,ApJ,433,65

O’Connell R.W.,Gallagher J.S.,Hunter D.A.,Colley W.N.1995,ApJ,446,L1 Telesco C.M.1988,ARA&A26,343

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