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Good afternoon, I need to get evolutionary tracks of star with different masses using this project, how can I do it?
And is it possible to get the names of evolutionary stages such as "Main Sequence"…
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### Routes
```routes
/springer/journal/:journal
```
### Full routes
```fullroutes
https://rsshub.app/springer/journal/40820
https://rsshub.app/springer/journal/41114
```
### Relat…
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The default hard upper limit for the temperatures should be increased from the current 7.0 if want to apply X-PSI for hot (e.g. bursting) neutron stars (at least if want to avoid making customized scr…
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Report: Had improved Neutron lasers on two white stars and two Shanteens all fully charged with double power for sustained firing. They are now all set for recharge after a single turn of firing.
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First of all, congratulations to v1.0!
I first had reported it upstream to the KDE Plasma developers, but I was asked to report it downstream instead.
### Expected Behaviour
Stellarium opens in …
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An improvement to our modelling of AGN and XRBs would be to use a Novikov-Thorne disk,
which does not have a hard inner boundary.
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This expected behavior
can result in UC being auto-detected when neutron stars are nex…
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Dear Keith...
I am evaluating the limits of your GDML tool with GMSH.
So, the initial conditions... I manually configurated path to GDML in FEM addon and restored check-box state.
![Screenshot…
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I read it with interest, some comments, mostly textual advice:
Line 10: "This yields varies" -> "These yields vary"
Line 11-13: I have a few comments about this part.
* What do you mean by a "…
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Third-Party Client Matrix Page: https://pulsar.apache.org/docs/next/client-libraries
1. Some clients are obsolete, they have not been updated for a long time, should we still show them?
2. What'…