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

In 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.

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Бібліографічні деталі
Опубліковано в: :Advances in Astronomy and Space Physics
Дата:2011
Автори: Malygin, M.G., Iakubovskyi, D.A.
Формат: Стаття
Мова:English
Опубліковано: Advances in astronomy and space physics 2011
Онлайн доступ:https://nasplib.isofts.kiev.ua/handle/123456789/118982
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Назва журналу:Digital Library of Periodicals of National Academy of Sciences of Ukraine
Цитувати:Search 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.

Репозитарії

Digital Library of Periodicals of National Academy of Sciences of Ukraine
id nasplib_isofts_kiev_ua-123456789-118982
record_format dspace
spelling Malygin, M.G.
Iakubovskyi, D.A.
2017-06-02T18:34:59Z
2017-06-02T18:34:59Z
2011
Search 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.
987-966-439-367-3
https://nasplib.isofts.kiev.ua/handle/123456789/118982
In 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.
M. 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.
en
Advances in astronomy and space physics
Advances in Astronomy and Space Physics
Search for cyclotron absorptions from magnetars in the quiescence with XMM-Newton
Article
published earlier
institution Digital Library of Periodicals of National Academy of Sciences of Ukraine
collection DSpace DC
title Search for cyclotron absorptions from magnetars in the quiescence with XMM-Newton
spellingShingle Search for cyclotron absorptions from magnetars in the quiescence with XMM-Newton
Malygin, M.G.
Iakubovskyi, D.A.
title_short Search for cyclotron absorptions from magnetars in the quiescence with XMM-Newton
title_full Search for cyclotron absorptions from magnetars in the quiescence with XMM-Newton
title_fullStr Search for cyclotron absorptions from magnetars in the quiescence with XMM-Newton
title_full_unstemmed Search for cyclotron absorptions from magnetars in the quiescence with XMM-Newton
title_sort search for cyclotron absorptions from magnetars in the quiescence with xmm-newton
author Malygin, M.G.
Iakubovskyi, D.A.
author_facet Malygin, M.G.
Iakubovskyi, D.A.
publishDate 2011
language English
container_title Advances in Astronomy and Space Physics
publisher Advances in astronomy and space physics
format Article
description In 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.
isbn 987-966-439-367-3
url https://nasplib.isofts.kiev.ua/handle/123456789/118982
citation_txt Search 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.
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