| Issue |
Title |
File |
| Vol 60, No 2 (2016) |
PN G068.1+11.0: A young pre-cataclysmic variable with an extremely hot primary |
|
|
Mitrofanova A.A., Shimansky V.V., Borisov N.V., Spiridonova O.I., Gabdeev M.M.
|
| Vol 62, No 12 (2018) |
Polarization of Gravitational Waves in General Teleparallel Theories of Gravity |
|
|
Hohmann M.
|
| Vol 63, No 11 (2019) |
Polarization Properties of Weakly Relativistic Cylindrical Jets |
|
|
Chernov S.V.
|
| Vol 63, No 1 (2019) |
Possible Electromagnetic Manifestations of Merging Black Holes |
|
|
Bisikalo D.V., Zhilkin A.G., Kurbatov E.P.
|
| Vol 60, No 11 (2016) |
Possible origins of the diversity of types of Active Galactic Nuclei |
|
|
Komberg B.V., Repin S.V.
|
| Vol 60, No 1 (2016) |
Possible reasons for the frequency splitting of the harmonics of type II solar radio bursts |
|
|
Eselevich V.G., Eselevich M.V., Zimovets I.V.
|
| Vol 61, No 5 (2017) |
Probing cosmic plasma with giant pulses from the crab nebula pulsar |
|
|
Rudnitskii A.G., Popov M.V., Soglasnov V.A.
|
| Vol 63, No 3 (2019) |
Profile of the 9.85-GHz Neutral Hydrogen Line Taking into Account the Zeeman Effect (Computations and Solar Observations) |
|
|
Dravskikh A.F., Peterova N.G., Topchilo N.A.
|
| Vol 61, No 4 (2017) |
Progress in low-frequency radio astronomy and I.S. Shklovskii’s contribution to its development |
|
|
Konovalenko A.A.
|
| Vol 61, No 2 (2017) |
Properties of the distribution of azimuthal magnetic field in a plasma flow during laboratory simulations of astrophysical jets in a plasma-focus installation |
|
|
Mitrofanov K.N., Krauz V.I., Myalton V.V., Vinogradov V.P., Kharrasov A.M., Vinogradova Y.V.
|
| Vol 62, No 12 (2018) |
Prospects for Strongly Lensed Supernovae Behind Hubble Frontier Fields Galaxy Clusters with the James Webb Space Telescope |
|
|
Petrushevska T., Okamura T., Kawamata R., Hangard L., Mahler G., Goobar A.
|
| Vol 62, No 3 (2018) |
Proton Flares in Solar Activity Complexes: Possible Origins and Consequences |
|
|
Isaeva E.S., Tomozov V.M., Yazev S.A.
|
| Vol 61, No 11 (2017) |
Pulsations in the atmospheres of hot Jupiters possessing magnetic fields |
|
|
Bisikalo D.V., Arakcheev A.S., Kaigorodov P.V.
|
| Vol 62, No 12 (2018) |
Radiation-Mediated Shocks: Kinetic Processes and Transition to Collisionless Shocks |
|
|
Derishev E.
|
| Vol 61, No 4 (2017) |
Radio galaxies of different populations on the Planck mission maps |
|
|
Verkhodanov O.V., Solovyov D.I., Ulakhovich O.S., Khabibullina M.L., Majorova E.K.
|
| Vol 63, No 3 (2019) |
Radio Sources in the Central Section of the RZF Catalog. Search for Objects with Ultra-Steep Spectra |
|
|
Pariiskii Y.N., Semenova T.A., Temirova A.V., Bursov N.N.
|
| Vol 61, No 4 (2017) |
RadioAstron and millimetron space observatories: Multiverse models and the search for life |
|
|
Kardashev N.S.
|
| Vol 61, No 4 (2017) |
RATAN-600 surveys and the cosmological gene of the universe |
|
|
Pariiskii Y.N., Verkhodanov O.V.
|
| Vol 61, No 11 (2017) |
Reduction of mass loss by the hot Jupiter WASP-12b due to its magnetic field |
|
|
Arakcheev A.S., Zhilkin A.G., Kaigorodov P.V., Bisikalo D.V., Kosovichev A.G.
|
| Vol 60, No 2 (2016) |
Refinement of the parameters of the binary pulsar B0655+64 based on 111 MHz observations |
|
|
Losovskii B.Y., Dumskii D.V., Logvinenko S.V.
|
| Vol 61, No 11 (2017) |
Refractive shift in the position of the pulsar PSR B0329+54, measured at 111, 610, and 2300 MHz |
|
|
Rodin A.E., Starovoit E.D.
|
| Vol 62, No 12 (2018) |
Regular Substructures in the Rich Open Galaxy Clusters |
|
|
Panko E.A., Andrievsky S.M., Yemelianov S.I., Stepaniuk A.M.
|
| Vol 61, No 1 (2017) |
Regularities in the response of spectral lines to small perturbations in physical quantities in the photosphere |
|
|
Mozharovskii S.G.
|
| Vol 63, No 12 (2019) |
Reheating Temperature from D-Term Cosmological Inflation Braneworld |
|
|
Salamate F., Khay I., Ferricha-Alami M., Chakir H., Bennai M.
|
| Vol 61, No 8 (2017) |
Relation between the parameters of dust and of molecular and atomic gas in extragalactic star-forming regions |
|
|
Smirnova K.I., Murga M.S., Wiebe D.S., Sobolev A.M.
|
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