Works matching IS 05717256 AND DT 2021 AND VI 64 AND IP 2
Results: 12
Higher-Dimensional Anisotropic Modified Holographic Ricci Dark Energy Cosmological Model in Lyra Manifold.
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- Astrophysics, 2021, v. 64, n. 2, p. 258, doi. 10.1007/s10511-021-09686-z
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Solutions for Massless Bosons in the Mannheim-Kazanas Space-Time.
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- Astrophysics, 2021, v. 64, n. 2, p. 244, doi. 10.1007/s10511-021-09685-0
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On the Formation of a Nonequilibrium Chemical Composition in the Shells of Neutron Stars.
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- Astrophysics, 2021, v. 64, n. 2, p. 228, doi. 10.1007/s10511-021-09684-1
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Multilayer Spherical Stellar Clusters with Uniform Density.
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- Astrophysics, 2021, v. 64, n. 2, p. 219, doi. 10.1007/s10511-021-09683-2
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Modulation of Galactic Cosmic Rays Due to Magnetic Clouds and Associated Structures in the Interplanetary Space: 1996-2018.
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- Astrophysics, 2021, v. 64, n. 2, p. 210, doi. 10.1007/s10511-021-09682-3
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Oxygen-Rich Cool Stars in the Cepheus Region. New Spectroscopic Observations of Selected Objects from the KP2001 Catalog.
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- Astrophysics, 2021, v. 64, n. 2, p. 203, doi. 10.1007/s10511-021-09681-4
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PV CEP and V350 CEP: Stars on the Way between FUors and EXors.
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- Astrophysics, 2021, v. 64, n. 2, p. 187, doi. 10.1007/s10511-021-09680-5
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Activity of Two Young Stars of Solar Type with Planetary Systems from the Ursa Major Moving Group of Stars and the Stream Psc-Eri.
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- Astrophysics, 2021, v. 64, n. 2, p. 178, doi. 10.1007/s10511-021-09679-y
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KIC 7732964 – A Possible Candidate FK Com-Type Star.
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- Astrophysics, 2021, v. 64, n. 2, p. 172, doi. 10.1007/s10511-021-09678-z
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New Orbit and Estimate of the Mass of the Star 61 Cygni Based on Observations of it in 1819-2019.
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- Astrophysics, 2021, v. 64, n. 2, p. 160, doi. 10.1007/s10511-021-09677-0
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Investigation of the Environmental Dependence of Galaxy Age in the CMASS Galaxy Sample of SDSS DR12.
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- Astrophysics, 2021, v. 64, n. 2, p. 150, doi. 10.1007/s10511-021-09676-1
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On the Problem of the Galaxy Alignment with Groups and Clusters.
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- Astrophysics, 2021, v. 64, n. 2, p. 141, doi. 10.1007/s10511-021-09675-2
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