Search for cyclotron absorptions from magnetars in the quiescence with XMM-Newton

dc.contributor.authorMalygin, M.G.
dc.contributor.authorIakubovskyi, D.A.
dc.date.accessioned2017-06-02T18:34:59Z
dc.date.available2017-06-02T18:34:59Z
dc.date.issued2011
dc.description.abstractIn this work, we perform the detailed analysis of absorption features in spectra of magnetar candidates observed by XMM-Newton satellite. No significant line-like feature has been found. This negative result may indicate the possible presence of smoothing out the absorption features mechanisms.uk_UA
dc.description.sponsorshipM. M. thanks to Lontkovskyi D. I. and Melnyk G. M. for helpful and fruitful discussions. All the data analysis has been processed using the computing facilities of the Virtual Roentgen and Gamma Observatory in Ukraine (http://virgo.org.ua). Both authors are grateful to McGill Pulsar Group for the inappreciated information placed here: http://www.physics.mcgill.ca/<sup>~</sup>pulsar/magnetar/main.html.uk_UA
dc.identifier.citationSearch for cyclotron absorptions from magnetars in the quiescence with XMM-Newton / M.G. Malygin, D.A. Iakubovskyi // Advances in Astronomy and Space Physics. — 2011. — Т. 1., вип. 1-2. — С. 43-46. — Бібліогр.: 20 назв. — англ.uk_UA
dc.identifier.isbn987-966-439-367-3
dc.identifier.urihttps://nasplib.isofts.kiev.ua/handle/123456789/118982
dc.language.isoenuk_UA
dc.publisherAdvances in astronomy and space physicsuk_UA
dc.relation.ispartofAdvances in Astronomy and Space Physics
dc.statuspublished earlieruk_UA
dc.titleSearch for cyclotron absorptions from magnetars in the quiescence with XMM-Newtonuk_UA
dc.typeArticleuk_UA

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