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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
Data sources: Datacite
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Extended far-UV emission surrounding AGB stars as seen by GALEX

descriptionPublicationkeyboard_double_arrow_right Conference object , Other literature type 10 Jan 2022Publisher:Zenodo
Authors: Rastau, Vlad; Mecina, Marko; Kerschbaum, Franz; Krebs, David; Drechsler, Marcel; Strottner, Xavier; Mulato, Lionel;

doi: 10.5281/zenodo.5834285 , 10.5281/zenodo.5834284

Extended far-UV emission surrounding AGB stars as seen by GALEX

Abstract

In a recent systematic Aladin survey of extended UV or IR emission structures associated with evolved AGB variables we came across several so far unknown extended features in GALEX FUV. These range from very faint, barely visible ones over arc-like features to large, well-defined rings or bubbles. Besides the FUV emission no comparable NUV counterpart was detected for any of the observed structures. This poster provides only a first overview of the objects for which a more detailed study is planned.

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Keywords

AGB stars, UV emission

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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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