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ZENODO
Dataset . 2021
Data sources: Datacite
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ZENODO
Dataset . 2021
Data sources: ZENODO
Claim

astroneb/WR_PN_Kinematic_Models: WR-PN-Kinematic-Models.1.1

Research datakeyboard_double_arrow_right Dataset 03 Sep 2021Publisher:Zenodo
Authors: Danehkar, Ashkbiz;

doi: 10.5281/zenodo.5410754

astroneb/WR_PN_Kinematic_Models: WR-PN-Kinematic-Models.1.1

Abstract

Morpho-kinematic properties of Wolf-Rayet planetary nebulae. Supplementary Data Figure 5. The interactive figure of the morpho-kinematic mesh models of the PNe M 3-30, Hb 4, IC 1297, Th 2-A, Pe 1-1, M 1-32, M 3-15, M 1-25, Hen 2-142, K 2-16, MGC 6578, M 2-42, NGC 6567 and NGC 6629. Citation @article{Danehkar2021, author = {{Danehkar}, A.}, title = {Morpho-kinematic properties of Wolf-Rayet planetary nebulae}, journal = {submitted (arXiv:2107.03994)}, volume = {}, number = {}, pages = {}, year = {2021}, doi = {} } Learn More GitPage: https://astroneb.github.io/WR_PN_Kinematic_Models/

Related Organizations
Keywords

kinematic, Wolf-Rayet, morphology, nebulae, planetary nebulae, ISM

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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!
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