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Transient Sources in Elliptical Galaxies

Authors: Brassington N.; Fabbiano G.; Kim D.; Zezas A.; Angelini L.; Davies R.; Fragos T.; +7 Authors

Transient Sources in Elliptical Galaxies

Abstract

A key observational result that can constrain the nature of Low-Mass X-ray binaries (LMXBs) is their time variability. From theory it has been suggested that transient behavior is expected from luminous (LX>10^37 erg/s) LMXBs if these sources have evolved from native X-ray binaries in the stellar field, whereas GC-LMXBs are only expected to display transient behavior at lower luminosities.

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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!
0
Average
Average
Average
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