К. А. Постнов

6.0k total citations · 1 hit paper
188 papers, 3.1k citations indexed

About

К. А. Постнов is a scholar working on Astronomy and Astrophysics, Geophysics and Nuclear and High Energy Physics. According to data from OpenAlex, К. А. Постнов has authored 188 papers receiving a total of 3.1k indexed citations (citations by other indexed papers that have themselves been cited), including 179 papers in Astronomy and Astrophysics, 42 papers in Geophysics and 34 papers in Nuclear and High Energy Physics. Recurrent topics in К. А. Постнов's work include Astrophysical Phenomena and Observations (112 papers), Pulsars and Gravitational Waves Research (105 papers) and Gamma-ray bursts and supernovae (75 papers). К. А. Постнов is often cited by papers focused on Astrophysical Phenomena and Observations (112 papers), Pulsars and Gravitational Waves Research (105 papers) and Gamma-ray bursts and supernovae (75 papers). К. А. Постнов collaborates with scholars based in Russia, Germany and United States. К. А. Постнов's co-authors include L. R. Yungelson, М. Е. Прохоров, N. I. Shakura, V. Lipunov, D. Klochkov, L. Hjalmarsdotter, A. Kochetkova, J. Wilms, М. С. Пширков and A. M. Cherepashchuk and has published in prestigious journals such as Nature, Physical Review Letters and SHILAP Revista de lepidopterología.

In The Last Decade

К. А. Постнов

170 papers receiving 2.9k citations

Hit Papers

align trajectories

What are hit papers?

Hit papers significantly outperform the citation benchmark for their cohort. A paper qualifies if it has ≥500 total citations, achieves ≥1.5× the top-1% citation threshold for papers in the same subfield and year (this is the minimum needed to enter the top 1%, not the average within it), or reaches the top citation threshold in at least one of its specific research topics.

The Evolution of Compact Binary Star Systems

2014 269 citations К. А. Постнов, L. R. Yungelson profile →

Peers

Countries citing papers authored by К. А. Постнов

Since Specialization

Citations

This map shows the geographic impact of К. А. Постнов's research. It shows the number of citations coming from papers published by authors working in each country. You can also color the map by specialization and compare the number of citations received by К. А. Постнов with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites К. А. Постнов more than expected).

Fields of papers citing papers by К. А. Постнов

Since Specialization

Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by К. А. Постнов. Nodes represent research fields, and links connect fields that are likely to share authors. Colored nodes show fields that tend to cite the papers produced by К. А. Постнов. The network helps show where К. А. Постнов may publish in the future.

Co-authorship network of co-authors of К. А. Постнов

This figure shows the co-authorship network connecting the top 25 collaborators of К. А. Постнов. A scholar is included among the top collaborators of К. А. Постнов based on the total number of citations received by their joint publications. Widths of edges represent the number of papers authors have co-authored together. Node borders signify the number of papers an author published with К. А. Постнов. К. А. Постнов is excluded from the visualization to improve readability, since they are connected to all nodes in the network.

All Works

Sort: Min cites: Since: Top N: Style:

20 of 20 papers shown

#	Work	Indexed citations
1	Unique microquasar SS433: new results, new issues 2025 ·Physics-Uspekhi ·A. M. Cherepashchuk, А. В. Додин, К. А. Постнов	2
2	Cyclical accretion regime change in the slow X-ray pulsar 4U 0114+65 observed with Chandra 2025 ·Astronomy and Astrophysics ·(unknown), (unknown), К. А. Постнов, (unknown), (unknown), (unknown), (unknown), (unknown)	0
3	Precision methods of pulsar timing and polarimetry: results and prospects 2024 ·Uspekhi Fizicheskih Nauk ·К. А. Постнов, N. K. Porayko, М. С. Пширков	0
4	Precision methods of pulsar timing and polarimetry: results and prospects 2024 ·Physics-Uspekhi ·К. А. Постнов, N. K. Porayko, М. С. Пширков	0
5	Spectroscopic searches for evolutionary orbital period changes in WR+OB binaries: The case of WR 127 (Hen 3-1772) 2024 ·Astronomy and Astrophysics ·(unknown), A. M. Cherepashchuk, А. В. Додин, К. А. Постнов	2
6	НАБЛЮДЕНИЯ МАССИВНЫХ СКОПЛЕНИЙ ГАЛАКТИК ИЗ ОБЗОРА ВСЕГО НЕБА ТЕЛЕСКОПА eРОЗИТА НА БОРТУ КОСМИЧЕСКОЙ ОБСЕРВАТОРИИ СРГ 2023 ·(unknown), (unknown), (unknown), M. Gilfanov, (unknown), (unknown), (unknown), А. В. Моисеев, (unknown), (unknown), (unknown), (unknown), К. А. Постнов, (unknown), А. А. Старобинский, (unknown), E. Churazov	0
7	The first mm detection of a neutron star high-mass X-ray binary 2023 ·Monthly Notices of the Royal Astronomical Society Letters ·J. van den Eijnden, L. Sidoli, (unknown), N. Degenaar, I. El Mellah, Felix Fürst, V. Grinberg, P. Kretschmar, S. Martínez‐Núñez, J. C. A. Miller‐Jones, К. А. Постнов, T. D. Russell	1
8	Elusive hot stripped helium stars in the Galaxy 2023 ·Astronomy and Astrophysics ·L. R. Yungelson, (unknown), К. А. Постнов, (unknown), L. M. Oskinova, W.‐R. Hamann	5
9	Discovery of orbital eccentricity and evidence for orbital period increase of SS433 2021 ·Monthly Notices of the Royal Astronomical Society Letters ·A. M. Cherepashchuk, A. Belinski, А. В. Додин, К. А. Постнов	20
10	Galactic population of black holes in detached binaries with low-mass stripped helium stars: the case of LB-1 (LS V+22 25) 2020 ·Monthly Notices of the Royal Astronomical Society Letters ·L. R. Yungelson, (unknown), К. А. Постнов, (unknown)	5
11	Modelling of 35-d superorbital cycle of B and V light curves of IMXB HZ Her/Her X-1 2020 ·Monthly Notices of the Royal Astronomical Society ·(unknown), N. I. Shakura, К. А. Постнов, (unknown), I. Bikmaev, (unknown), R. Staubert, J. Wilms, (unknown), (unknown), S. Yu. Shugarov, (unknown), (unknown), G. Schönherr, A. Schwope, D. Klochkov	3
12	Mass ratio in SS433 revisited 2019 ·Monthly Notices of the Royal Astronomical Society ·A. M. Cherepashchuk, К. А. Постнов, A. Belinski	15
13	Wind-accreting symbiotic X-ray binaries 2019 ·Monthly Notices of the Royal Astronomical Society ·L. R. Yungelson, (unknown), К. А. Постнов	27
14	Black hole spins in coalescing binary black holes 2018 ·Monthly Notices of the Royal Astronomical Society ·К. А. Постнов, (unknown)	20
15	Do we see accreting magnetars in X-ray pulsars? 2014 ·Springer Link (Chiba Institute of Technology) ·К. А. Постнов, N. I. Shakura, A. Kochetkova, L. Hjalmarsdotter	7
16	Long-term change in the cyclotron line energy in Hercules X-1 2014 ·Springer Link (Chiba Institute of Technology) ·R. Staubert, D. Klochkov, J. Wilms, К. А. Постнов, N. I. Shakura, R. E. Rothschild, Felix Fürst, Fiona A. Harrison	23
17	Quenching of the strong aperiodic accretion disk variability at themagnetospheric boundary 2009 ·Springer Link (Chiba Institute of Technology) ·M. Revnivtsev, E. Churazov, К. А. Постнов, Sergey S. Tsygankov	59
18	INTEGRAL observations of Hercules X-1 2008 ·Springer Link (Chiba Institute of Technology) ·D. Klochkov, R. Staubert, К. А. Постнов, N. I. Shakura, A. Santangelo, Sergey S. Tsygankov, A. Lutovinov, I. Kreykenbohm, J. Wilms	27
19	First simultanous \nX-ray and optical observations of rapid variability of supercritical accretor SS433 2004 ·Springer Link (Chiba Institute of Technology) ·M. Revnivtsev, R. Burenin, S. Fabrika, К. А. Постнов, I. Bikmaev, M. Pavlinsky, R. Sunyaev, I. Khamitov, (unknown)	8
20	Presence of a Quadrupole Component of the Magnetic Field Near the Surface of the Neutron Star in HERCULES-X-1 1991 ·N. I. Shakura, К. А. Постнов, М. Е. Прохоров	0

Rankless uses publication and citation data sourced from OpenAlex, an open and comprehensive bibliographic database. While OpenAlex provides broad and valuable coverage of the global research landscape, it—like all bibliographic datasets—has inherent limitations. These include incomplete records, variations in author disambiguation, differences in journal indexing, and delays in data updates. As a result, some metrics and network relationships displayed in Rankless may not fully capture the entirety of a scholar's output or impact.

Explore authors with similar magnitude of impact