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期刊详情
Astronomy Reports
IF
0.7
论文数
31
被引数
2133
相关解读
0
订阅
期刊论文
31
相关解读
0
期刊论文
31
发表时间
发表时间
IF
被引数
Outer and Inner Orbits of the Bright Doubly Eclipsing System BU CMi
ASTRONOMY REPORTS
IF
0.7
2025-11-01
0
PRE
AI
Volkova, A. S.; Volkov, I. M.
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Some Limits on Optical Emission of Fast Radio Bursts
ASTRONOMY REPORTS
IF
0.7
2025-11-01
0
OA
AI
Chasovnikov, A. R.; Lipunov, V. M.; Vlasenko, D. M.; Zhirkov, K. K.; Tyurina, N. V.
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Relationship between Poincaré Sections and Spectral Characteristics of Orbits of Globular Clusters in the Central Region of the Galaxy
ASTRONOMY REPORTS
IF
0.7
2025-11-01
0
PRE
AI
Bajkova, A. T.; Smirnov, A. A.; Bobylev, V. V.
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Multicolor Transit Photometry: Searching for Traces of Exoplanet Atmospheres
ASTRONOMY REPORTS
IF
0.7
2025-11-01
0
PRE
AI
Bekesov, E. V.; Lyzenko, K. A.; Cherepashchuk, A. M.; Belinski, A. A.; Shugarov, S. Yu.; Tatarnikov, A. M.; Maslennikova, N. A.
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Correction for Observational Selection Effects of the Samples of Low-Mass Exoplanets Discovered with the Radial Velocity Technique
ASTRONOMY REPORTS
IF
0.7
2025-11-01
0
PRE
AI
Ananyeva, V. I.; Shashkova, I. A.; Tavrov, A. V.
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The Pushchino Multibeams Pulsar Search. VII. The Results of the Timing of 12 Slow Pulsars
ASTRONOMY REPORTS
IF
0.7
2025-11-01
0
PRE
AI
Andrianov, S. A.; Potapov, V. A.; Tyul'bashev, S. A.
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Writhing of the Axes of Eruptive Prominences at the Late Stage of Eruption
ASTRONOMY REPORTS
IF
0.7
2025-11-01
0
OA
AI
Filippov, B. P.
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The Distribution of Young Spectroscopic Binary Stars by Masses and by Mass Ratio of the Components Corrected for Observational Selection Effects
ASTRONOMY REPORTS
IF
0.7
2025-11-01
0
PRE
AI
Eretnova, O. V.; Dremova, G. N.; Tarasova, D. V.
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Formation of Large-Scale Structures of the Universe: Singularities and Evolution in Pressureless Media
ASTRONOMY REPORTS
IF
0.7
2025-11-01
0
PRE
AI
Aptekarev, A. I.; Kalashnikov, I. Yu.; Rykov, Yu. G.; Chechetkin, V. M.
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Do Planets Affect the Behavior of the Long-term Solar Activity?
ASTRONOMY REPORTS
IF
0.7
2025-11-01
0
PRE
AI
Katsova, M.; Obridko, V.; Sokoloff, D.; Emelyanov, N.
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The Pushchino Multibeam Pulsar Search. VI. Method for Pulsar Timing Using Poorly Timed Data
ASTRONOMY REPORTS
IF
0.7
2025-11-01
0
PRE
AI
Andrianov, S. A.; Potapov, V. A.; Tyul'bashev, S. A.; Logvinenko, S. V.; Oreshko, V. V.
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An Analysis of Equilibrium Points in the Sitnikov Square Configuration with Oblate Primaries
ASTRONOMY REPORTS
IF
0.7
2025-11-01
0
PRE
AI
Ullah, M. Shahbaz; Idrisi, M. Javed
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Critical Accretion to Neutron Star with an Evaluation of Nucleosynthesis
ASTRONOMY REPORTS
IF
0.7
2025-11-01
0
PRE
AI
Aksenov, A. G.; Chechetkin, V. M.
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Ic-Photometry of the X-Ray Nova GS 2000+25 (QZ Vul): Orbital Light Curve Modeling and Black Hole Mass
ASTRONOMY REPORTS
IF
0.7
2025-11-01
0
PRE
AI
Cherepashchuk, A. M.; Khruzina, T. S.; Atapin, K. E.
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Equilibrium Structures and Stability in Radiating Oblate Binary Systems with Heterogeneity
ASTRONOMY REPORTS
IF
0.7
2025-11-01
0
PRE
AI
Idrisi, M. Javed; Keshav; Masih, Advin
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First Results of the Operation of the RCO-500 Optical Station of the Russian-Cuban Observatory
ASTRONOMY REPORTS
IF
0.7
2025-11-01
0
PRE
AI
Naroenkov, S. A.; Nalivkin, M. A.; Tarasenkov, A. N.; Sysolina, Yu. V.; Savanov, I. S.; Sachkov, M. E.; Rodrigues, O. Pons; Fonseca, Z. Barcena
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Three Models of the Gravitational Potential of the Milky Way
银河系引力势的三种模型
ASTRONOMY REPORTS
IF
0.7
2025-10-01
0
PRE
AI
Bobylev, V. V.; Bajkova, A. T.; Smirnov, A. A.
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RRAT Search on Declinations from+42° to+55° with a Neural Network
使用神经网络对赤纬+42°至+55°范围进行RRAT搜索
ASTRONOMY REPORTS
IF
0.7
2025-10-01
0
PRE
AI
Eldarov, I. V.; Tyul'bashev, S. A.; Kitaeva, M. A.; Tyul'basheva, G. E.
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Influence of Gas Elemental Composition on Molecular Kinetics
气体元素组成对分子动力学的影响
ASTRONOMY REPORTS
IF
0.7
2025-10-01
0
PRE
AI
Vorobyov, O. P.; Vasiliev, E. O.
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SU UMa-type Dwarf Nova MASTER OT J212624.16+253827.2 in the Period Gap: Orbital Period and Negative Superhumps
SU UMa型矮新星MASTER OT J212624.16+253827.2位于周期间隙中:轨道周期和负超丘
ASTRONOMY REPORTS
IF
0.7
2025-10-01
1
PRE
AI
Pavlenko, E. P.; Sosnovskij, A. A.; Antonyuk, K. A.; Kolbin, A. I.; Antonyuk, O. I.
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