Works matching IS 05717256 AND DT 2016 AND VI 59 AND IP 1
Results: 13
Addition Laws for Intensities of Radiation Emerging from Scattering Atmospheres Containing Energy Sources.
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- Astrophysics, 2016, v. 59, n. 1, p. 11, doi. 10.1007/s10511-016-9411-3
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Possible Reasons for the Slow Rotation of BF Ori.
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- Astrophysics, 2016, v. 59, n. 1, p. 20, doi. 10.1007/s10511-016-9412-2
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Fractality of Isotherms of the Cosmic Microwave Background Based on Data from the Planck Spacecraft.
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- Astrophysics, 2016, v. 59, n. 1, p. 31, doi. 10.1007/s10511-016-9413-1
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Photometric Analysis of the Eclipsing Binaries with Eccentric Orbits GSC 4277 0586=V0898 Cep and GSC 4481 0230=V0922 Cep.
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- Astrophysics, 2016, v. 59, n. 1, p. 38, doi. 10.1007/s10511-016-9414-0
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Spectral Characteristics of Radiation from the Nucleus of the Seyfert Galaxy NGC 1275 After an Epoch of its Maximum Activity.
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- Astrophysics, 2016, v. 59, n. 1, p. 48, doi. 10.1007/s10511-016-9415-z
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Distribution of Pulsars in the Galaxy.
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- Astrophysics, 2016, v. 59, n. 1, p. 57, doi. 10.1007/s10511-016-9416-y
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Analysis of UBV-Photometric Observations of the Massive, Early-Type Binary System V729 Cyg (Cyg OB2 No. 5).
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- Astrophysics, 2016, v. 59, n. 1, p. 68, doi. 10.1007/s10511-016-9417-x
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Gravitational Radiation of Compact Stars.
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- Astrophysics, 2016, v. 59, n. 1, p. 80, doi. 10.1007/s10511-016-9418-9
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Magnetic Field of Strange Dwarfs.
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- Astrophysics, 2016, v. 59, n. 1, p. 90, doi. 10.1007/s10511-016-9419-8
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Comparative Analysis of the Activity Cycles of the Atmospheres of the Sun and of Stars of the Solar-Type.
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- Astrophysics, 2016, v. 59, n. 1, p. 101, doi. 10.1007/s10511-016-9420-2
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Internal Radiation Field in the Nonlinear Transfer Problem for a One-Dimensional Anisotropic Medium. I.
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- Astrophysics, 2016, v. 59, n. 1, p. 114, doi. 10.1007/s10511-016-9421-1
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Properties and Formation of Star Clusters.
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- Astrophysics, 2016, v. 59, n. 1, p. 126, doi. 10.1007/s10511-016-9422-0
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Isentropic 'Shock Waves' in Numerical Simulations of Astrophysical Problems.
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- Astrophysics, 2016, v. 59, n. 1, p. 1, doi. 10.1007/s10511-016-9410-4
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