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Evidence for a binary origin of a central compact object

A non-pulsating neutron star in the supernova remnant HESS J1731-347/G353.6-0.7 with a carbon atmosphere HESS J1731-347/G353.6-0.7 shows no pulsations and exhibits a blackbody-like X-ray spectrum

The neutron star in HESS? J1731 - 347: Central compact objects as laboratories to study the equation of state of superdense matter

Evidence for a binary origin of a central compact object

A non-pulsating neutron star in the supernova remnant HESS J1731-347/G353.6-0.7 with a carbon atmosphere HESS J1731-347/G353.6-0.7 shows no pulsations and exhibits a blackbody-like X-ray spectrum

The neutron star in HESS? J1731 - 347: Central compact objects as laboratories to study the equation of state of superdense matter

The direct cooling tail method for X-ray burst analysis to constrain neutron star masses and radii

Black holes, gravitational waves and fundamental physics: A roadmap

Николай Страхов и Иоганн Готлиб Фихте

Пересечения максимальных θ-подгрупп, содержащих формационные радикалы пересечения θ, Ф() G G F всех максимальных θ-подгрупп конечной группы , Gсодержащих . G

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