reformating

AaronDavidSchneider · Nov 22, 2023 · e4a4ccf · e4a4ccf
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@@ -30,82 +30,44 @@ Adjust paths in `chemcomp/helper/main_helper` if you need different directories
 ## Publications
 ### Original Publications
 
--   
+-   [Schneider & Bitsch (2021a)](https://ui.adsabs.harvard.edu/abs/2021A&A...654A..71S)</br>
+    How drifting and evaporating pebbles shape giant planets. I. Heavy element content and atmospheric C/O
 
-    [Schneider & Bitsch (2021a)](https://ui.adsabs.harvard.edu/abs/2021A&A...654A..71S)
+-   [Schneider & Bitsch (2021b)](https://ui.adsabs.harvard.edu/abs/2021A&A...654A..72SS)</br>
+    How drifting and evaporating pebbles shape giant planets. II. Volatiles and refractories in atmospheres
 
-    :   How drifting and evaporating pebbles shape giant planets. I.
-        Heavy element content and atmospheric C/O
-
--   
-
-    [Schneider & Bitsch (2021b)](https://ui.adsabs.harvard.edu/abs/2021A&A...654A..72SS)
-
-    :   How drifting and evaporating pebbles shape giant planets. II.
-        Volatiles and refractories in atmospheres
-
--   
-
-    [Bitsch, Schneider & Kreidberg (2022)](https://ui.adsabs.harvard.edu/abs/2022A&A...665A.138B)
-
-    :   How drifting and evaporating pebbles shape giant planets. III.
-        The formation of WASP-77A b and $\tau$ Boötis b
+-   [Bitsch, Schneider & Kreidberg (2022)](https://ui.adsabs.harvard.edu/abs/2022A&A...665A.138B)</br>
+    How drifting and evaporating pebbles shape giant planets. III. The formation of WASP-77A b and $\tau$ Boötis b
 
 Please cite [Schneider & Bitsch(2021a)](https://ui.adsabs.harvard.edu/abs/2021A&A...654A..71S), if you use `chemcomp` in your work.
 
 ### Publications using `chemcomp`
 
--   
-
-    [Bitsch et al. (2021)](https://ui.adsabs.harvard.edu/abs/2021A&A...649L...5B)
-
-    :   Dry or water world? How the water contents of inner sub-Neptunes
-        constrain giant planet formation and the location of the water
-        ice line
-
--   
-
-    [Hühn & Bitsch (2023)](https://ui.adsabs.harvard.edu/abs/2023A&A...676A..87H)
-
-    :   How accretion of planet-forming disks influences stellar
-        abundances
-
--   
-
-    [Bitsch & Mah (2023)](https://ui.adsabs.harvard.edu/abs/2023arXiv230900509B)
-
-    :   Enriching inner discs and giant planets with heavy elements
-
--   
-
-    [Mah & Bitsch (2023a)](https://ui.adsabs.harvard.edu/abs/2023A&A...673A..17M)
-
-    :   Forming super-Mercuries: Role of stellar abundances
-
--   
-
-    [Mah & Bitsch (2023b)](https://ui.adsabs.harvard.edu/abs/2023A&A...677L...7M)
-
-    :   Close-in ice lines and the super-stellar C/O ratio in discs
-        around very low-mass stars
+-   [Bitsch et al. (2021)](https://ui.adsabs.harvard.edu/abs/2021A&A...649L...5B)</br>
+    Dry or water world? How the water contents of inner sub-Neptunes constrain giant planet formation and the location of the water ice line
 
--   
+-   [Hühn & Bitsch (2023)](https://ui.adsabs.harvard.edu/abs/2023A&A...676A..87H)</br>
+    How accretion of planet-forming disks influences stellar abundances
 
-    [Savvidou & Bitsch (2023)](https://ui.adsabs.harvard.edu/abs/2023arXiv230903807S)
+-   [Bitsch & Mah (2023)](https://ui.adsabs.harvard.edu/abs/2023arXiv230900509B)</br>
+    Enriching inner discs and giant planets with heavy elements
 
-    :   How to make giant planets via pebble accretion
+-   [Mah & Bitsch (2023a)](https://ui.adsabs.harvard.edu/abs/2023A&A...673A..17M)</br>
+    Forming super-Mercuries: Role of stellar abundances
 
--   
+-   [Mah & Bitsch (2023b)](https://ui.adsabs.harvard.edu/abs/2023A&A...677L...7M)</br>
+    Close-in ice lines and the super-stellar C/O ratio in discs around very low-mass stars
 
-    [Danti, Bitsch & Mah (2023)](https://ui.adsabs.harvard.edu/abs/2023arXiv231002886D)
+-   [Savvidou & Bitsch (2023)](https://ui.adsabs.harvard.edu/abs/2023arXiv230903807S)</br>
+    How to make giant planets via pebble accretion
 
-    :   Composition of giant planets: the roles of pebbles and
-        planetesimals
+-   [Danti, Bitsch & Mah (2023)](https://ui.adsabs.harvard.edu/abs/2023arXiv231002886D)</br>
+    Composition of giant planets: the roles of pebbles and planetesimals
 
 And several more in preperation (last updated: 22.11.2023)
 
 
 ## Thanks:
 - I would like to thank Bertram Bitsch for his enormous support during the development of this code and for continuing to use the code together with his students.
 - I would like to thank Cornelis Dullemond for providing the solver which (in adapted version) is used to solve the gas viscous disk equation and dust transport equation.
-- I would like to thank everyone, who has already used chemcomp in their work and has contributed in fixing small bugs.
+- I would like to thank everyone, who has already used chemcomp in their work and has contributed in fixing small bugs.