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https://doi.org/10.1063/1.3250...
Article . 2009 . Peer-reviewed
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https://dx.doi.org/10.1063/1.3...
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Neutron Star Model Atmospheres

descriptionPublicationkeyboard_double_arrow_right Article , Other literature type 01 Jan 2009Publisher:AIPJournal:AIP Conference Proceedings
Authors: Valery Suleimanov; Thomas Rauch; Klaus Werner; Alexander Y. Potekhin; Juri Poutanen; Ivan Hubeny; James M. Stone; +2 Authors

doi: 10.1063/1.3250076

Neutron Star Model Atmospheres

Abstract

Determination of neutron star (NS) parameters is an important astrophysical problem. The stellar radius depends on the mass and the equation of state (EOS) in the NS core, which is not well known. Therefore, with masses and radii inferred from observations we are able to select between various theories for the EOS. Theoretical models of NS spectra are needed for this purpose.

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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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