Results 11 to 20 of about 389,431 (321)
Microscopic Vortex Velocity in the Inner Crust and Outer Core of Neutron Stars [PDF]
, 2016 Treatment of the vortex motion in the superfluids of the inner crust and the outer core of neutron stars is a key ingredient in modeling a number of pulsar phenomena, including glitches and magnetic field evolution.
Alpar, M. Ali, Gügercinoğlu, Erbil
core +2 more sources
PALEOEARTHQUAKES IN THE PRIBAIKALIE: METHODS AND RESULTS OF DATING
Геодинамика и тектонофизика, 2015 In the Pribaikalie and adjacent territories, seismogeological studies have been underway for almost a half of the century and resulted in discovery of more than 70 dislocations of seismic or presumably seismic origin.
Oleg P. Smekalin +2 more
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Evaluation of the self-similarity of earthquake epicenters field in the Baikal region
Литосфера, 2019 Object of research. The mathematical apparatus of the theory of fractals and the algorithms developed within its framework are used to assess the statistical self-similarity of the fields of epicenter earthquakes in the Baikal region.Materials and ...
A. V. Klyuchevskii +2 more
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Геодинамика и тектонофизика, 2018 Our study aimed to clarify the seismic potential of the Severobaikalsk fault and to discover the structural features of active faults on the NW shores of Lake Baikal.
O. V. Lunina +3 more
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mBio, 2020 The crust is the outermost spore layer of most Bacillus strains devoid of an exosporium. This outermost layer, composed of both proteins and carbohydrates, plays a major role in the adhesion and spreading of spores into the environment.
Thomas Dubois +9 more
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Геодинамика и тектонофизика, 2018 Seismic hazard assessment with the use of an integrated approach is discussed on the case of the left bank of the Angara river in Irkutsk, Russia. Potential earthquake focal zones have been identified in the study area.
A. Yu. Eskin +3 more
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Continued cooling of the crust in the neutron star low-mass X-ray binary KS 1731-260 [PDF]
, 2010 Some neutron star low-mass X-ray binaries have very long outbursts (lasting several years) which can generate a significant amount of heat in the neutron star crust. After the system has returned to quiescence, the crust then thermally relaxes.
Arnaud +12 more
core +3 more sources
Non-radial Oscillation Modes of Compact Stars with a Crust [PDF]
, 2017 Oscillation modes of isolated compact stars can, in principle, be a fingerprint of the equation of state (EoS) of dense matter. We study the non-radial high-frequency l=2 spheroidal modes of neutron stars and strange quark stars, adopting a two-component
Flores, C. Vasquez +2 more
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Известия высших учебных заведений: Геология и разведка, 2015 The article considers the results of integrated engineering geological studies of Proterozoic sandstones at the construction site near the town of Udokan.
T. G. Ryashchenko +3 more
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