tag:blogger.com,1999:blog-2094985635923554000.post7166565820025797679..comments2023-09-30T17:36:30.328+01:00Comments on A cluster of thoughts: How to make a star clusterAnonymoushttp://www.blogger.com/profile/16914018869228807140noreply@blogger.comBlogger3125tag:blogger.com,1999:blog-2094985635923554000.post-8713915813322722762022-06-07T10:19:08.892+01:002022-06-07T10:19:08.892+01:00This comment has been removed by the author.Anonymousnoreply@blogger.comtag:blogger.com,1999:blog-2094985635923554000.post-5712064983239152922016-11-24T12:07:12.365+00:002016-11-24T12:07:12.365+00:00I think kinematics both for ejected stars but also...I think kinematics both for ejected stars but also for very young clusters could provide some good insights into this.<br /><br />I've also wondered whether there might be anything learnt from the typical timescales on which filaments exist before star formation occurs in them - i.e. do they live long enough for collisions between filaments to occur and channel gas into a dense clustered configuration?Anonymoushttps://www.blogger.com/profile/16914018869228807140noreply@blogger.comtag:blogger.com,1999:blog-2094985635923554000.post-50875843127284474892016-11-24T11:15:50.362+00:002016-11-24T11:15:50.362+00:00Excellent! It's where we were trying to go wit...Excellent! It's where we were trying to go with Carla's thesis, but along the GP to get better statistics. <br />If it's the second of these mechanisms, then you'd need to get rid of a lot of potential energy to form the cluster - could be done with the gas but you might expect some stars to be kicked out ⇒ RV studies to look for high velocity stars? Antonionoreply@blogger.com