Physics – Atomic Physics
Scientist
Physics
Atomic Physics
Scientist
Ioffe Phys.-Tech. Institute, St.-Petersburg
Ioffe Phys.-Tech. Inst., St. Petersburg
Ioffe Inst., St.-Petersburg
Ioffe Phys.-Tech. Institute http: / / www.ioffe.rssi.ru / ;
Ioffe Phys.-Tech. Inst., St. Petersburg;
Ioffe Inst., St.Petersburg
Ioffe Institute, St. Petersburg
Ioffe Physical-Technical Institute, Saint Petersburg, Russia
Ioffe Phys.-Tech. Inst., Saint-Petersburg;
Ioffe Phys.-Tech. Inst., St.-Petersburg;
Ioffe Physical-Technical Institute, St. Petersburg, Russia
Ioffe Physical-Technical Institute, Saint-Petersburg
Centre de Recherche Astrophysique de Lyon
Ioffe Physico-Technical Institute
CRAL, ENS-Lyon
Ioffe Phys.-Tech. Inst., St. Petersburg, Russia;
Ioffe Institute, St.Petersburg
Ioffe Inst., St. Petersburg
Ioffe Phys.-Tech. Institute, St. Petersburg;
Ioffe Institute, St.-Petersburg
Ioffe Institute, St. Petersburg;
Ioffe Phys.-Tech. Inst., St.Petersburg
Nordita, Copenhagen
Ioffe Phys.-Tech. Inst., St.Petersburg;
ENS-Lyon, CRAL
Ioffe Physico-Technical Institute, Russian Federation
Ioffe Physical Technical Institute, Politekhnicheskaya 26, 194021, Saint-Petersburg, Russia
Ioffe Physical-Technical Institute
Ioffe Physico-Technical Institute, 194021 St. Petersburg, Russia
Ioffe Physical-Technical Institute, Politekhnicheskaya Str., 26, St. Petersburg, 194021, Russia; CRAL, École Normale Supérieure de Lyon, UMR CNRS No. 5574, Université de Lyon, 69364, Lyon Cedex 07, France; Isaac Newton Institute of Chile, St. Petersburg Branch, Russia
Ioffe Physical-Technical Institute, Polytekhnicheskaya str. 26, St. Petersburg 194021, Russia
Ioffe Physico-Technical Institute, Politekhnicheskaya 26, St. Petersburg 194021, Russia
(Erratum) Electron conduction along quantizing magnetic fields in neutron star crusts. I. Theory.
(Erratum) Electron conduction along quantizing magnetic fields in neutron star crusts. II. Practical formulae.
Addendum to "Equation of state of classical Coulomb plasma mixtures"
Analytical representations of unified equations of state of neutron-star matter
Atmospheres and Spectra of Strongly Magnetized Neutron Stars -- III. Partially Ionized Hydrogen Models
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