Quote:
Originally Posted by Stonius
Fascinating. So, assuming that the gas cloud has some of the heavier elements, it could be a newborn CG of Population I stars. I looked up the wikipedia entry on R136 because you peaked my interest. I particularly found the following passage interesting;
"R136 produces most of the energy that makes the Tarantula Nebula visible. The estimated mass of the cluster is 450,000 solar masses, suggesting it may become a globular cluster in the future. [...] The cluster R136 contains many of the most massive and luminous stars known, including R136a1. Within the central 5 parsecs there are 32 of the hottest type O stars (O2.0–3.5), 40 other O stars, and 12 Wolf-Rayet stars, mostly of the extremely luminous WNh type. Within 150 parsecs there are a further 325 O stars and 19 Wolf-Rayet stars."
Markus
|
Maybe it is 2 million years old? Trying to remember back a few years so my globular cluster research
The same thing is happening at the centre of M42 where the trapezium is what lights up near all of the Orion Nebula.