User talk:86.8.202.14

Globular clusters
In the article on globular clusters you added the following entry:


 * On the other hand, these claims of intermediate mass black holes have met with some skepticism. The heaviest objects in globular clusters are expected to sink to the cluster center due to mass segregation. These will be white dwarfs and neutron stars in an old stellar population like a globular cluster. As pointed out in two papers by Holger Baumgardt and collaborators, the mass-to-light ratio should rise sharply towards the center of the cluster, even without a black hole, in both M15 and G1.

Can you find some citations for the statements that the heaviest objects will be white dwarfs and neutron stars, as well as the two papers by Holger Baumgardt? Thank you. :-) &mdash; RJH (talk) 18:59, 13 September 2006 (UTC)


 * Thank you! &mdash; RJH (talk) 22:34, 13 September 2006 (UTC)

October 2021
Hello, I'm Fbergo. I wanted to let you know that one or more of your recent contributions&#32;to Morhad Amdouni have been undone because they did not appear constructive. If you would like to experiment, please use the sandbox. If you have any questions, you can ask for assistance at the Teahouse. Thanks. Fbergo (talk) 14:11, 20 October 2021 (UTC)