Works matching DE "ROCHE equipotentials"
Results: 116
Accretion onto Black Holes. II.
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- Astronomy Reports, 2024, v. 68, p. S19, doi. 10.1134/S1063772924701105
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THE CRITICAL MASS RATIO FOR W UMA-TYPE CONTACT BINARY SYSTEMS.
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- Serbian Astronomical Journal, 2024, n. 209, p. 55, doi. 10.2298/SAJ2409055E
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Tidal decay and stable Roche-lobe overflow of short-period gaseous exoplanets.
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- Celestial Mechanics & Dynamical Astronomy, 2016, v. 126, n. 1-3, p. 227, doi. 10.1007/s10569-016-9704-1
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The Potential and Equipotentiality of Spacecraft.
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- Cosmic Research, 2004, v. 42, n. 1, p. 32, doi. 10.1023/B:COSM.0000017559.84665.90
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Kepler Kataloğundan Seçilen Üç W UMa Tipi Değen Çift Yıldızın (KIC3732732, KIC3936357 ve KIC10802917) Işık Eğrisi Analizleri.
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- Journal of the Institute of Science & Technology / Iğdır Üniversitesi Fen Bilimleri Enstitüsü Dergisi, 2022, v. 12, n. 2, p. 735, doi. 10.21597/jist.1054191
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Thyroid Agenesis: A Case Report with Review of Literature.
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- World Journal of Endocrine Surgery, 2012, v. 4, n. 3, p. 99, doi. 10.5005/jp-journals-10002-1107
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A Two-Dimensional Hydrostatically Equilibrium Atmosphere of a Neutron Star with Given Differential Rotation.
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- Astronomy Letters, 2000, v. 26, n. 12, p. 788, doi. 10.1134/1.1331159
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Entorhinal Tau Pathology, Episodic Memory Decline, and Neurodegeneration in Aging.
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- Journal of Neuroscience, 2018, v. 38, n. 3, p. 530, doi. 10.1523/JNEUROSCI.2028-17.2017
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On the Use of Roche Equipotentials in Analysing the Problems of Binary and Rotating Stars.
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- Journal of Astrophysics & Astronomy, 2013, v. 34, n. 1, p. 69, doi. 10.1007/s12036-013-9168-6
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Post-Common-Envelope Binaries with Distorted Secondaries.
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- Astrophysics & Space Science, 2005, v. 296, n. 1-4, p. 481, doi. 10.1007/s10509-005-4898-9
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The Evolution of Massive Close Binaries.
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- Astrophysics & Space Science, 2005, v. 296, n. 1-4, p. 337, doi. 10.1007/s10509-005-4846-8
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Light Curve Analysis of Early-Type Overcontact Systems.
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- Astrophysics & Space Science, 2005, v. 296, n. 1-4, p. 255, doi. 10.1007/s10509-005-4466-3
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Global Solution of Dynamical Systems a Report to Z. Kopal, on what Followed Since.
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- Astrophysics & Space Science, 2005, v. 296, n. 1-4, p. 79, doi. 10.1007/s10509-005-4383-5
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Adoption of Extended Dupuit-Forchheimer Assumptions to Non-Darcy Flow Problems.
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- Transport in Porous Media, 2016, v. 113, n. 3, p. 457, doi. 10.1007/s11242-016-0703-1
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Solar system: Recipe for making Saturn's rings.
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- Nature, 2010, v. 468, n. 7326, p. 903, doi. 10.1038/nature09738
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System of Roche-Coordinates for Stellar Model Distorted by Differential Rotation.
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- International Transactions in Mathematical Sciences & Computer, 2010, v. 3, n. 2, p. 331
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Robust Hybrid Algorithm of PSO and SOCP for Grating Lobe Suppression and against Array Manifold Mismatch.
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- Radioengineering, 2018, v. 27, n. 4, p. 1128, doi. 10.13164/re.2018.1128
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The double-degenerate, super-Chandrasekhar nucleus of the planetary nebula Henize 2-428.
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- Nature, 2015, v. 519, n. 7541, p. 63, doi. 10.1038/nature14124
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W 50 Morphology and the Dynamics of SS 433 Formation—The Origin of TeV Gammas from the Microquasar.
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- Particles (2571-712X), 2024, v. 7, n. 3, p. 805, doi. 10.3390/particles7030047
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Aeronomy of the Atmosphere of Ultra-Hot Jupiter Kelt9b with Allowance for the Kinetics of Hydrogen Atom Levels.
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- Astronomy Reports, 2024, v. 68, n. 8, p. 802, doi. 10.1134/S1063772924700732
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The Evolutionary Status of the Galaxy's X-ray Binary Stars.
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- Astronomy Reports, 2024, v. 68, n. 6, p. 565, doi. 10.1134/S1063772924700562
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Evolution of the X-ray Binary System Sco X-1.
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- Astronomy Reports, 2023, v. 67, n. 11, p. 1074, doi. 10.1134/S1063772923100049
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Parameters of X-Ray Binary Sco X-1 in the Model of Partial Filling of Roche Lobe by Optical Star.
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- Astronomy Reports, 2022, v. 66, n. 4, p. 348, doi. 10.1134/S1063772922040023
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Evolution of the X-ray Binary System Sco X-1 within the Framework of the Induced Stellar Wind Model.
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- Astronomy Reports, 2022, v. 66, n. 11, p. 925, doi. 10.1134/S1063772922100055
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MHD Model of the Interaction of a Coronal Mass Ejection with the Hot Jupiter HD 209458b.
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- Astronomy Reports, 2021, v. 65, n. 8, p. 676, doi. 10.1134/S1063772921090092
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Destruction of a Star during the Evolution of a Star + Supermassive Black Hole System.
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- Astronomy Reports, 2021, v. 65, n. 2, p. 95, doi. 10.1134/S1063772921020025
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Coronal Mass Ejection Effect on Envelopes of Hot Jupiters.
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- Astronomy Reports, 2020, v. 64, n. 2, p. 159, doi. 10.1134/S1063772920020055
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Features of the Flow Structure in the Vicinity of the Inner Lagrangian Point in Polars.
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- Astronomy Reports, 2018, v. 62, n. 8, p. 492, doi. 10.1134/S1063772918080024
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Pulsations in the atmospheres of hot Jupiters possessing magnetic fields.
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- Astronomy Reports, 2017, v. 61, n. 11, p. 925, doi. 10.1134/S1063772917110026
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Reduction of mass loss by the hot Jupiter WASP-12b due to its magnetic field.
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- Astronomy Reports, 2017, v. 61, n. 11, p. 932, doi. 10.1134/S1063772917110014
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The evolution of stars paired with supermassive black holes.
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- Astronomy Reports, 2017, v. 61, n. 8, p. 663, doi. 10.1134/S1063772917070095
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The mass of the black hole in the X-ray binary LMC X-1.
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- Astronomy Reports, 2016, v. 60, n. 12, p. 1029, doi. 10.1134/S1063772916120015
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Estimation of the accuracy of methods for determining component masses for low-mass X-ray binary systems.
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- Astronomy Reports, 2017, v. 61, n. 1, p. 1, doi. 10.1134/S1063772917010012
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Mass-loss rates of 'hot-Jupiter' exoplanets with various types of gaseous envelopes.
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- Astronomy Reports, 2014, v. 58, n. 10, p. 679, doi. 10.1134/S1063772914100047
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Wolf-Rayet stars with relativistic companions.
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- Astronomy Reports, 2013, v. 57, n. 9, p. 657, doi. 10.1134/S1063772913090084
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<i>K</i>-Corrections to radial-velocity curves of optical components in X-ray binaries. Massive systems with weak X-ray heating.
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- Astronomy Reports, 2013, v. 57, n. 9, p. 669, doi. 10.1134/S1063772913090047
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Orbital-period variations in the eclipsing binary Y Cam.
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- Astronomy Reports, 2013, v. 57, n. 7, p. 517, doi. 10.1134/S1063772913060024
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Synthetic light curves of close binaries in a cool-disk model. The 'hot line' and 'hot spot' as visual indicators of interaction between the flow and disk.
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- Astronomy Reports, 2011, v. 55, n. 5, p. 425, doi. 10.1134/S1063772911050039
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The mass of the black hole in the X-ray binary M33 X-7 and the evolutionary status of M33 X-7 and IC 10 X-1.
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- Astronomy Reports, 2009, v. 53, n. 3, p. 232, doi. 10.1134/S1063772909030056
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Formation of a radiative wind and accretion disk in microquasars. Generation of flare activity in the disk due to an increase in the supply of material to the Lagrange point L<sub>1</sub>. The system LMC X-3.
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- Astronomy Reports, 2008, v. 52, n. 1, p. 40, doi. 10.1134/S1063772908010058
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The mass of the compact object in the low-mass X-ray binary 2S 0921-630.
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- Astronomy Reports, 2006, v. 50, n. 7, p. 544, doi. 10.1134/S1063772906070043
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Hydrodynamical Modeling of Circularization in Close Binary Systems in Early Stages of Their Evolution on the Dynamical Time Scale.
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- Astronomy Reports, 2005, v. 49, n. 11, p. 892, doi. 10.1134/1.2127993
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Photometric analysis on RZ Horologii: An evolved and active Algol with a δ Scuti component.
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- Publications of the Astronomical Society of Japan, 2023, v. 75, n. 4, p. 732, doi. 10.1093/pasj/psad033
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Mass flows and their behaviors in the SS 433–W 50 system.
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- Publications of the Astronomical Society of Japan, 2022, v. 74, n. 4, p. 991, doi. 10.1093/pasj/psac050
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Is there a low-mass triple system orbiting around the massive semi-detached binary ZZ Cassiopeiae?
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- Publications of the Astronomical Society of Japan, 2022, v. 74, n. 3, p. 533, doi. 10.1093/pasj/psac016
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SX Piscium: A near-contact mass-transferring binary with a possible brown dwarf companion.
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- Publications of the Astronomical Society of Japan, 2019, v. 71, n. 5, p. N.PAG, doi. 10.1093/pasj/psz086
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Mass-transfer properties of overcontact systems in the Kepler eclipsing binary catalog.
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- Publications of the Astronomical Society of Japan, 2018, v. 70, n. 5, p. N.PAG, doi. 10.1093/pasj/psy086
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Repeated short-term spectral softening in the low/hard state of the Galactic black hole candidate Swift J1753.5−0127.
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- Publications of the Astronomical Society of Japan, 2015, v. 67, n. 1, p. 1
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Embryonic muscle development in direct and indirect developing marine flatworms (Platyhelminthes, Polycladida).
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- Evolution & Development, 2009, v. 11, n. 3, p. 290, doi. 10.1111/j.1525-142X.2009.00331.x
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Error propagation for three common height-system corrections to differential levelling.
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- Journal of Spatial Science, 2011, v. 56, n. 1, p. 39, doi. 10.1080/14498596.2011.567410
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