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Gijs Nelemans

@gijsnelemans.bsky.social

✨ πŸ”­ Astronomer πŸ’₯ πŸ’» | Binary stars πŸ’«| Gravitational Waves γ€°οΈπŸŒŠ|

106 Followers  |  123 Following  |  5 Posts  |  Joined: 30.11.2024  |  1.7881

Latest posts by gijsnelemans.bsky.social on Bluesky

Beneden alle peil

21.12.2024 09:29 β€” πŸ‘ 1    πŸ” 0    πŸ’¬ 0    πŸ“Œ 0

If all we are probing with current observations is BHs formed since z~1 the mass growth is limited. I fully agree it is a big stretch, but I would like to find even better arguments.

01.12.2024 16:32 β€” πŸ‘ 2    πŸ” 0    πŸ’¬ 1    πŸ“Œ 0

I’m not sure. Binary BH formation could be inefficient at early times and the LVK systems all originated relatively recently. The GW only probe a tiny fraction of the mass in BH, so it is easier to argue around it I would think

01.12.2024 15:48 β€” πŸ‘ 2    πŸ” 0    πŸ’¬ 1    πŸ“Œ 0

Problem with the examples so far (as far as I can see) is that they are small numbers, so there is wiggle room (exotic formation, observational bias etc). I'm quite sure this cannot be true, but we need one (or more) killer argument that this simply cannot be true...

01.12.2024 14:39 β€” πŸ‘ 2    πŸ” 0    πŸ’¬ 1    πŸ“Œ 0

Also, all stellar BH formed early in galaxies would become quite massive. A quick calculation for the Milky Way shows that the O(10^7) BHs would have masses up to 5000Msun with total mass 2.3e10Msun! I thought it would be dead easy to rule that out, but haven't found a killer argument yet...

01.12.2024 14:27 β€” πŸ‘ 2    πŸ” 0    πŸ’¬ 1    πŸ“Œ 0
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I often show my students this visualization of how atmospheric COβ‚‚ travels around the globe. Our attitude toward burning fossil fuels would change significantly if we could actually see COβ‚‚.

svs.gsfc.nasa.gov/goto?11719

29.11.2024 22:09 β€” πŸ‘ 1213    πŸ” 493    πŸ’¬ 52    πŸ“Œ 22

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