Powered by OpenAIRE graph
Found an issue? Give us feedback
image/svg+xml art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos Open Access logo, converted into svg, designed by PLoS. This version with transparent background. http://commons.wikimedia.org/wiki/File:Open_Access_logo_PLoS_white.svg art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos http://www.plos.org/ ZENODOarrow_drop_down
image/svg+xml art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos Open Access logo, converted into svg, designed by PLoS. This version with transparent background. http://commons.wikimedia.org/wiki/File:Open_Access_logo_PLoS_white.svg art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos http://www.plos.org/
ZENODO
Audiovisual . 2025
License: CC BY
Data sources: ZENODO
ZENODO
Audiovisual . 2025
License: CC BY
Data sources: Datacite
ZENODO
Audiovisual . 2025
License: CC BY
Data sources: Datacite
 View all 2 versions
Claim

Videos of simulations from Afruni et al. 2025: 'The long life of ultra diffuse galaxies inside low-density dark matter halos: the case of AGC 114905'

appsOther research productkeyboard_double_arrow_right Audiovisual 11 Feb 2025Publisher:Zenodo
Authors: Afruni, Andrea;

doi: 10.5281/zenodo.14852153 , 10.5281/zenodo.14852154

Videos of simulations from Afruni et al. 2025: 'The long life of ultra diffuse galaxies inside low-density dark matter halos: the case of AGC 114905'

Abstract

Videos of the stellar and gas components for all the simulations performed in Afruni et al. 2025, entitled: 'The long life of ultra diffuse galaxies inside low-density dark matter halos: the case of AGC 114905'. The naming convention is 'Video_component_proj_type_sim.avi', with: - component = Stellar/Gas; type of component - proj = edgeon/faceon; type of projection - type = hydro/Nbody; simulation with or without hydrodynamics, see the manuscript for more details - sim = Case1/Case2/noDM/Case3; galaxy model, see the manuscript for more details

Related Organizations
  • BIP!
    Impact byBIP!
    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).
    		 0
    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.
    		 Average
    influence
    This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
    		 Average
    impulse
    This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
    		 Average
Powered by OpenAIRE graph
Found an issue? Give us feedback
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
Average
Average
Average