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Article . 2011
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Chandra HRC confirms that M15 X-2 is the currently flaring source in M15

descriptionPublicationkeyboard_double_arrow_right Article 01 Jan 2011 Netherlands English
Authors: Sivakoff, G.R.; Heinke, C.O.; Miller-Jones, J.C.A.; Altamirano, D.; Kuulkers, E.; Morii, M.;

handle: 11245/1.357784

Chandra HRC confirms that M15 X-2 is the currently flaring source in M15

Abstract

Radio observations of the ongoing X-ray flare in the globular cluster M15 (ATel #3356, #3363), suggested that the ultracompact X-ray binary M15 X-2 was the flaring source (ATel #3378). This is surprising as ultracompact X-ray binaries such as M15 X-2 (22 minute period, Dieball et al. 2005, ApJ, 634, L105) are generally not expected to show factors of >10 flux variations over timescales of days to weeks.

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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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