Stochastic background of gravitational waves emitted by magnetars
Two classes of high-energy sources in our galaxy are believed to host magnetars, ie neutron
stars whose emission results from the dissipation of their magnetic field. The extremely high …
stars whose emission results from the dissipation of their magnetic field. The extremely high …
[引用][C] Stochastic background of gravitational waves emitted by magnetars
S Marassi, R Ciolfi, R Schneider, L Stella… - Monthly Notices of the …, 2010 - cir.nii.ac.jp
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情報学研究所 学術情報ナビゲータ[サイニィ] 詳細へ移動 検索フォームへ移動 論文・データをさがす …
Stochastic background of gravitational waves emitted by magnetars
S Marassi, R Ciolfi, R Schneider, L Stella… - arXiv preprint arXiv …, 2010 - arxiv.org
Two classes of high energy sources in our galaxy are believed to host magnetars, neutron
stars whose emission results from the dissipation of their magnetic field. The extremely high …
stars whose emission results from the dissipation of their magnetic field. The extremely high …
[引用][C] Stochastic background of gravitational waves emitted by magnetars
S MARASSI, R CIOLFI, R SCHNEIDER… - Monthly notices of …, 2011 - pascal-francis.inist.fr
Stochastic background of gravitational waves emitted by magnetars CNRS Inist Pascal-Francis
CNRS Pascal and Francis Bibliographic Databases Simple search Advanced search Search …
CNRS Pascal and Francis Bibliographic Databases Simple search Advanced search Search …
Stochastic background of gravitational waves emitted by magnetars
S Marassi, R Ciolfi, R Schneider, L Stella… - … NOTICES OF THE …, 2011 - iris.uniroma1.it
Two classes of high-energy sources in our galaxy are believed to host magnetars, ie neutron
stars whose emission results from the dissipation of their magnetic field. The extremely high …
stars whose emission results from the dissipation of their magnetic field. The extremely high …
Stochastic background of gravitational waves emitted by magnetars
S Marassi, R Ciolfi, R Schneider, L Stella… - Monthly Notices of the …, 2011 - infona.pl
Two classes of high‐energy sources in our galaxy are believed to host magnetars, ie
neutron stars whose emission results from the dissipation of their magnetic field. The …
neutron stars whose emission results from the dissipation of their magnetic field. The …
[PDF][PDF] Stochastic background of gravitational waves emitted by magnetars
S Marassi, R Ciolfi, R Schneider, V Ferrari - 2010 - academia.edu
Two classes of high energy sources in our galaxy are believed to host magnetars, neutron
stars whose emission results from the dissipation of their magnetic field. The extremely high …
stars whose emission results from the dissipation of their magnetic field. The extremely high …
Stochastic background of gravitational waves emitted by magnetars
S Marassi, R Ciolfi, R Schneider… - Monthly Notices of the …, 2011 - ieeexplore.ieee.org
Two classes of high-energy sources in our galaxy are believed to host magnetars, ie neutron
stars whose emission results from the dissipation of their magnetic field. The extremely high …
stars whose emission results from the dissipation of their magnetic field. The extremely high …
Stochastic background of gravitational waves emitted by magnetars
S Marassi, R Ciolfi, R Schneider… - Monthly Notices of …, 2011 - ui.adsabs.harvard.edu
Two classes of high-energy sources in our galaxy are believed to host magnetars, ie neutron
stars whose emission results from the dissipation of their magnetic field. The extremely high …
stars whose emission results from the dissipation of their magnetic field. The extremely high …
Stochastic background of gravitational waves emitted by magnetars
S Marassi, R Ciolfi, R Schneider, L Stella… - Mon. Not. Roy. Astron …, 2011 - inspirehep.net
Two classes of high energy sources in our galaxy are believed to host magnetars, neutron
stars whose emission results from the dissipation of their magnetic field. The extremely high …
stars whose emission results from the dissipation of their magnetic field. The extremely high …