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Radiografia di un pasto stellare

descriptionPublicationkeyboard_double_arrow_right Other literature type 01 Jan 2018 Italian Publisher:Media Inaf
Authors: Matteo Boni;

doi: 10.20371/inaf/2724-2641/1663201

Radiografia di un pasto stellare

Abstract

Osservazioni ai raggi X della stella RW Aur A, nella costellazione del Toro, potrebbero spiegare il misterioso oscuramento periodico della stella come il risultato di successivi pasti a base di resti di giovani pianeti che si sono scontrati nelle sue vicinanze. Lo studio su The Astronomical Journal

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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
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