Timeline for Galactic rotation speed and density research
Current License: CC BY-SA 4.0
12 events
when toggle format | what | by | license | comment | |
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Oct 27, 2023 at 10:26 | comment | added | Rémy Galli | @xzczd Sorry, I have no mean to recover this trial : I scratched it ! | |
Oct 27, 2023 at 9:26 | review | Close votes | |||
Nov 9, 2023 at 3:07 | |||||
Oct 27, 2023 at 9:12 | vote | accept | Rémy Galli | ||
Oct 27, 2023 at 9:08 | comment | added | xzczd♦ |
Please show us your failed trial so we can diagnose. As mentioned in my last comment, my solution just works fine on the new vc according to my test.
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Oct 27, 2023 at 8:46 | history | edited | Rémy Galli | CC BY-SA 4.0 |
added 89 characters in body
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Oct 27, 2023 at 3:07 | comment | added | Alex Trounev |
@RémyGalli In a case of our Galaxy the density has a singular part $m\delta(R)$, where $m$ is the black hole mass (see Nobel prize 2020). Therefore equation for vc[R] should be update.
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Oct 27, 2023 at 1:42 | comment | added | xzczd♦ |
1. Please add the link to that "solutions given elswhere" to the body of your question. 2. My solution under your previous question fully applys to this new vc , which part are you having difficulty? (Of course you need to supplement the missing data at R==0 . )
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Oct 26, 2023 at 18:06 | answer | added | Ulrich Neumann | timeline score: 3 | |
Oct 26, 2023 at 17:27 | comment | added | Rémy Galli | @ Ulrich Yes,you are right and I noticed these two points but I cant find something working. with this Interpolating function. .... | |
Oct 26, 2023 at 17:03 | comment | added | Ulrich Neumann |
Have a look at the transformed integral equation. The expression v[R]^2/(4Pi R^2) must be finite for all values of R.
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Oct 26, 2023 at 16:51 | comment | added | Ulrich Neumann |
Your new dataset doesn't contain point R=0 !
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Oct 26, 2023 at 16:04 | history | asked | Rémy Galli | CC BY-SA 4.0 |