-
Numerous laboratory, heliospheric, and astrophysical plasmas are weakly ionized or partially ionized. Examples include stellar chromospheres, protoplanetary disks, molecular clouds, the cold neutral …
-
1.2 Checklist
- [x] 1 new planet for Wall
- Also move everything on a really inclined orbit and give Nyarlathotep a polar ring
- [ ] 2 new planets for Eon
- [ ] 8 new moons for Newell
…
-
reported by: @CloudyLex
we should look into this
```
Title:
Cosmic-ray and X-ray Heating of Interstellar Clouds and Protoplanetary Disks
Authors:
Glassgold, Alfred E.; Galli, Daniele; Padovani,…
-
I'm attempting to fit an SED of a star + protoplanetary disk. The attached image shows my current best effort, which is somewhat nonsensical.
1. The wavelength axis has to be in Angstroms, because tha…
-
Sir,
I am working on my M.Sc. thesis on protoplanetary discs and I have obtained following issues.
When running the segment of code given in "docs-->example_dust-->Dust_model.ipynb" to get an image…
-
We now have the initial components of an escape model integrated into PROTEUS. However, it is possible that accretion is also contemporaneous with magma ocean evolution. It would be interesting to exp…
-
reported by: @CloudyLex
```
Title:
The photodissociation and chemistry of CO isotopologues: applications to interstellar clouds and circumstellar disks
Authors:
Visser, R.; van Dishoeck, E. F.; B…
-
reported by: @CloudyLex
arXiv:1305.1781v1 [astro-ph.GA] 8 May 2013
```
Photodissociation of interstellar N2
Xiaohu Li1, Alan N. Heays1;2;3, Ruud Visser4, Wim Ubachs3, Brenton R. Lewis5, Stephen T.…
-
Object type "emission and reflection nebula is only used for the orion complex: M42, IC 427, IC 428.
It recommended to delete this object type and to change Orion complex to H-II area.
Simimar, objec…
-
We should restrict the scope to evaporating globules and knots. That is, excluding blister flows and champagne flows
So the main categories of ionized photoevaporation flows are:
1. In H II regi…