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Conference object . 2022
License: CC BY
Data sources: Datacite
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Other literature type . 2022
License: CC BY
Data sources: ZENODO
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Conference object . 2022
License: CC BY
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The newest born-again planetary nebula

descriptionPublicationkeyboard_double_arrow_right Conference object , Other literature type 04 Sep 2022Publisher:Zenodo
Authors: Molina, Borja Montoro; Guerrero, M.A.; Pérez-Díaz, B.; , J.A.Toalá; Cazzoli, Sara; Bertolami, M.M Miller; Morisset, C.;

doi: 10.5281/zenodo.7048799 , 10.5281/zenodo.7048798

The newest born-again planetary nebula

Abstract

HuBi 1 is the latest addition to the small but potentially not-so-strange group of born-again planetary nebulae. The VLTP suffered by its central star attenuated its magnitude by 10 mag in just 50 years, as well as giving it a unique inverted ionization structure. The recently measured ejecta reaching up to 200 km/s together with the aforementioned oddities made it the perfect candidate for a born-again nebula in the absence of confirmed ejecta abundances. We present the abundances of recent ejecta calculated using the MAPPINGS V code in a shock scenario as well as their main optical properties.

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selected citations
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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).
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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.
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