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cloudy
cloudy
Commits
9d622692
Commit
9d622692
authored
Oct 14, 2022
by
Chatzikos, Marios
Browse files
Merge branch 'NewDayDawns' into 'master'
New day dawns See merge request
!46
parents
47622384
87fdcf8c
Changes
2
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docs/latex/hazy1/federico-respini-sYffw0LNr7s-unsplash.pdf
0 → 100644
View file @
9d622692
File added
docs/latex/hazy1/hazy1.tex
View file @
9d622692
...
...
@@ -41,7 +41,7 @@ Hazy\\
\begin{figure}
\begin{center}
\hspace*
{
-1cm
}
\includegraphics
[clip=on,width=\columnwidth,height=0.6\textheight,keepaspectratio]
{
cooling-flow-spectrum-hazy1
}
\includegraphics
[clip=on,width=\columnwidth,height=0.6\textheight,keepaspectratio]
{
federico-respini-sYffw0LNr7s-unsplash
}
\end{center}
\end{figure}
...
...
@@ -63,16 +63,8 @@ Hazy\\
\noindent
{
\small
{
\em
Cover image:
The X-ray spectrum of a unit-volume parcel of gas cooling under conditions
of constant pressure (isobarically) from X-ray temperatures (1~keV), computed
at three resolving powers.
In the top panel, the resolving power is comparable the proposed
{
\it
Athena
}
resolving power around 6~keV.
In the bottom panel, the resolving power is comparable to the
{
\it
Chandra
}
non-dispersive resolving power around 1~keV.
In the middle panel, the resolving power is at the code default.
This functionality is new to
\Cloudy
, and it is described in
\citet
{
Chatzikos2015
}
, and Section~
\ref
{
sec:Cooling-Heating-NonEq
}
below.
The dawn of a new day, representing Cloudy's migration between
development platforms and new development plans. Photo by Federico Respini on Unsplash.
}
}
\clearpage
...
...
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