Experimental browser for the Atmosphere
4/4 Theoretical models are calibrated on well-studied clusters, where direct star counts in central regions (with telescopes such as Hubble) confirm the indirect estimates. These data help validate IMF and dynamical models for similar clusters. (You're welcome!)
May 7, 2025, 1:22 PM
{ "uri": "at://did:plc:5odp2okktic3ychbdqiw3kxi/app.bsky.feed.post/3lolikbqvhk2e", "cid": "bafyreib6y6ozpliopn26pwv6bzgkcrjcqbnh2zl24e5f5wbwgy2vfqxnwi", "value": { "text": "4/4\nTheoretical models are calibrated on well-studied clusters, where direct star counts in central regions (with telescopes such as Hubble) confirm the indirect estimates. These data help validate IMF and dynamical models for similar clusters.\n\n(You're welcome!)", "$type": "app.bsky.feed.post", "langs": [ "en" ], "reply": { "root": { "cid": "bafyreibqs7k246q2n4ppi4fciawxbcewiqakjalumueb75kz7y4hmr5oty", "uri": "at://did:plc:5odp2okktic3ychbdqiw3kxi/app.bsky.feed.post/3lojyrxnzjk2c" }, "parent": { "cid": "bafyreigdyngbgtcdesbvpoqw5y6ihk24q2zswoi43zr44ni5iyaglgs4lu", "uri": "at://did:plc:5odp2okktic3ychbdqiw3kxi/app.bsky.feed.post/3lolikbquic2e" } }, "createdAt": "2025-05-07T13:22:36.890Z" } }