From 80b32a51bd7bce53cb2a25139367be15c0abcc71 Mon Sep 17 00:00:00 2001 From: Michael Zingale Date: Sun, 1 Dec 2024 12:11:34 -0500 Subject: [PATCH] fix ref --- sphinx_docs/source/refs.bib | 4 ++-- sphinx_docs/source/transport.rst | 2 +- 2 files changed, 3 insertions(+), 3 deletions(-) diff --git a/sphinx_docs/source/refs.bib b/sphinx_docs/source/refs.bib index 15cd3999d..760f3b80c 100644 --- a/sphinx_docs/source/refs.bib +++ b/sphinx_docs/source/refs.bib @@ -626,10 +626,10 @@ @misc{autodiff year = {2018} } -@ARTICLE{timmes:2000, +@ARTICLE{timmes:2000b, author = {{Timmes}, F.~X.}, title = "{Physical Properties of Laminar Helium Deflagrations}", - journal = {\apj}, + journal = {APJ}, keywords = {HYDRODYNAMICS, METHODS: NUMERICAL, NUCLEAR REACTIONS, NUCLEOSYNTHESIS, ABUNDANCES, STARS: INTERIORS, Hydrodynamics, Methods: Numerical, nuclear reactions, nucleosynthesis; abundances, Stars: Interiors}, year = 2000, month = jan, diff --git a/sphinx_docs/source/transport.rst b/sphinx_docs/source/transport.rst index 32de39a9c..d1537c6e3 100644 --- a/sphinx_docs/source/transport.rst +++ b/sphinx_docs/source/transport.rst @@ -64,7 +64,7 @@ There are several implementations of the conductivity currently: * ``stellar`` : - This is a general stellar conductivity based on :cite:`timmes:2000`. + This is a general stellar conductivity based on :cite:`timmes:2000b`. It combines radiative opacities and thermal conductivities into a single expression. This conductivity is suitable for modeling laminar flames.