mirror of
https://git.lyx.org/repos/lyx.git
synced 2024-11-09 18:31:04 +00:00
aa_sample: cosmetics.
This commit is contained in:
parent
0a68c7cb3c
commit
0013389864
@ -43,8 +43,8 @@
|
||||
\use_package stackrel 1
|
||||
\use_package stmaryrd 1
|
||||
\use_package undertilde 1
|
||||
\cite_engine basic
|
||||
\cite_engine_type default
|
||||
\cite_engine natbib
|
||||
\cite_engine_type authoryear
|
||||
\biblio_style plain
|
||||
\use_bibtopic false
|
||||
\use_indices false
|
||||
@ -512,7 +512,7 @@ literal "true"
|
||||
|
||||
\end_inset
|
||||
|
||||
), originally used to study the Cepheı̈d pulsation mechanism, will be briefly
|
||||
), originally used to study the Cepheïd pulsation mechanism, will be briefly
|
||||
reviewed.
|
||||
The resulting stability criteria will be rewritten in terms of local state
|
||||
variables, local timescales and constitutive relations.
|
||||
@ -1203,7 +1203,7 @@ For solar composition gas the
|
||||
dissociation and the combined H, first He ionization zone, as indicated
|
||||
by vibrational instability.
|
||||
These regions of instability are much larger in extent and degree of instabilit
|
||||
y than the second He ionization zone that drives the Cepheı̈d pulsations.
|
||||
y than the second He ionization zone that drives the Cepheïd pulsations.
|
||||
|
||||
\end_layout
|
||||
|
||||
@ -1243,7 +1243,7 @@ status open
|
||||
Note:
|
||||
\series default
|
||||
If you cannot see the bibliography in the output, assure that you have
|
||||
gievn the full path to the Bib\SpecialChar TeX
|
||||
given the full path to the Bib\SpecialChar TeX
|
||||
style file
|
||||
\family sans
|
||||
aa.bst
|
||||
|
Loading…
Reference in New Issue
Block a user