Importance of Compton scattering for radiation spectra of isolated neutron stars

dc.contributor.author	Suleimanov V.
dc.contributor.author	Werner K.
dc.date.accessioned	2018-09-18T20:01:59Z
dc.date.available	2018-09-18T20:01:59Z
dc.date.issued	2007
dc.identifier.issn	0004-640X
dc.identifier.uri	https://dspace.kpfu.ru/xmlui/handle/net/135910
dc.description.abstract	Model atmospheres of isolated neutron stars with low magnetic field are calculated with Compton scattering taking into account. Radiation spectra computed with Compton scattering are softer than computed with Thomson scattering at high energies (E>5 keV) for hot (T eff>10 6 K) atmospheres with hydrogen-helium composition. Compton scattering is more significant to models with low surface gravity. Compton scattering is less important to models with solar abundance of heavy elements. © Springer Science+Business Media B.V. 2007.
dc.relation.ispartofseries	Astrophysics and Space Science
dc.subject	Atmospheres
dc.subject	Neutron stars
dc.subject	Radiative transfer
dc.subject	Scattering
dc.subject	X-rays
dc.title	Importance of Compton scattering for radiation spectra of isolated neutron stars
dc.type	Article
dc.relation.ispartofseries-issue	1-4
dc.relation.ispartofseries-volume	308
dc.collection	Публикации сотрудников КФУ
dc.relation.startpage	471
dc.source.id	SCOPUS0004640X-2007-308-14-SID34248137449

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