The s-process at Subsolar Metallicity: Insights from High-Resolution Infrared Spectroscopy of Magellanic Cloud Planetary Nebulae
Authors/Creators
-
1.
University of West Georgia
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2.
The University of Texas at Austin
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3.
Los Alamos National Laboratory
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4.
Konkoly Observatory
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5.
Monash University
- 6. University of Hull
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7.
Instituto de Astrofísica de Canarias
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8.
Georgia Institute of Technology
Description
# Data release
Here we present extra data for the article titled `The s-process at Subsolar
Metallicity: Insights from High-Resolution Infrared Spectroscopy of Magellanic
Cloud Planetary Nebulae`. There are two subdirectories:
## figures
The `figures` directory contains a subdirectory for each PN with the figures
in pdf format with the best fits of each model type for the given PNe with all
reasonable combinations of anchor elements.
## tables
The `tables` directory contains the tables in `tex` format that correspond
to each figure in the `figures` directory, with the difference that any model
above 50% GoF is printed out, with a minimum of one model per group (Monash,
Fruity, NuGrid). Inside of this directory, there is an additional directory:
`tables/plaintext_format`, which contains the same tables but in ASCII format
for parsing purposes.
LA-UR-26-23249
Files
Files
(1.9 MB)
| Name | Size | Download all |
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md5:3214cf7e5471ad8476b027261609bd88
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1.9 MB | Download |