From e4a4ccf008cf2897e2e142f5edf3372d3e71c863 Mon Sep 17 00:00:00 2001 From: Aaron David Schneider Date: Wed, 22 Nov 2023 09:40:59 +0100 Subject: [PATCH] reformating --- README.md | 80 +++++++++++++++---------------------------------------- 1 file changed, 21 insertions(+), 59 deletions(-) diff --git a/README.md b/README.md index 18aa496..1bb12ad 100755 --- a/README.md +++ b/README.md @@ -30,77 +30,39 @@ 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)
+ 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)
+ 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)
+ 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)
+ 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 - [Savvidou & Bitsch (2023)](https://ui.adsabs.harvard.edu/abs/2023arXiv230903807S) +- [Bitsch & Mah (2023)](https://ui.adsabs.harvard.edu/abs/2023arXiv230900509B)
+ 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)
+ 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 - [Danti, Bitsch & Mah (2023)](https://ui.adsabs.harvard.edu/abs/2023arXiv231002886D) +- [Savvidou & Bitsch (2023)](https://ui.adsabs.harvard.edu/abs/2023arXiv230903807S)
+ 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)
+ Composition of giant planets: the roles of pebbles and planetesimals And several more in preperation (last updated: 22.11.2023) @@ -108,4 +70,4 @@ 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. \ No newline at end of file +- I would like to thank everyone, who has already used chemcomp in their work and has contributed in fixing small bugs.