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ZENODO
Software . 2025
License: http://www.gnu.org/licenses/gpl-3.0-standalone.html
Data sources: ZENODO
ZENODO
Software . 2025
License: https://www.gnu.org/licenses/gpl-3.0-standalone.html
Data sources: Datacite
ZENODO
Software . 2025
License: https://www.gnu.org/licenses/gpl-3.0-standalone.html
Data sources: Datacite
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The Inflow with Ram Pressure Stripping galactic chemical evolution model

integration_instructionsResearch softwarekeyboard_double_arrow_right Software 20 Jan 2025 English Publisher:Zenodo
Authors: Kvasova, Katie;

doi: 10.5281/zenodo.14690724 , 10.5281/zenodo.14690723

The Inflow with Ram Pressure Stripping galactic chemical evolution model

Abstract

To improve our understanding on how alpha-elements evolve in a dwarf galaxy, we present a new analytical galactic chemical evolution model (GCE), which includes both gas inflow and environmentally caused gas loss. The model's name is Inflow with Ram Pressure Stripping (IRPS). The software consists of a Jupyter Notebook, which implements the solutions and contains illustrative examples on some properties of the IRPS.

Related Organizations
Keywords

Galactic astronomy, galactic chemical evolution

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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
0
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