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after a few million years the cluster will experience its first core-collapse supernovae, which will also expel gas from the vicinity.
birkaç milyon yıl sonra yıldız kümesi ilk çekirdek çökme süpernovasını tecrübe eder, bu da etraftaki gazları uzaklaştırır.
==external links==* atom smashers shed light on supernovae, big bang "sky & telescope online", april 22, 2005
==dış bağlantılar==* atom smashers shed light on supernovae, big bang "sky & telescope online", 22 nisan 2005
== see also ==* new general catalogue (ngc)* ngc 1365, spiral galaxy== external links ==* hst: celestial composition* ho et al., bvri photometry of supernovae*ngc 3370 at esa/hubble*astronomy picture of the day, 12 oct 2008==references==
== ayrıca bakınız ==* ngc 1365== dış bağlantılar ==* hst: celestial composition* ho et al., bvri photometry of supernovae* ngc 3370 at esa/hubble* astronomy picture of the day, 12 oct 2008== kaynaklar ==