S. P. Owocki

10.3k total citations · 1 hit paper
200 papers, 6.7k citations indexed

About

S. P. Owocki is a scholar working on Astronomy and Astrophysics, Computational Mechanics and Instrumentation. According to data from OpenAlex, S. P. Owocki has authored 200 papers receiving a total of 6.7k indexed citations (citations by other indexed papers that have themselves been cited), including 190 papers in Astronomy and Astrophysics, 20 papers in Computational Mechanics and 12 papers in Instrumentation. Recurrent topics in S. P. Owocki's work include Stellar, planetary, and galactic studies (147 papers), Astrophysics and Star Formation Studies (131 papers) and Solar and Space Plasma Dynamics (55 papers). S. P. Owocki is often cited by papers focused on Stellar, planetary, and galactic studies (147 papers), Astrophysics and Star Formation Studies (131 papers) and Solar and Space Plasma Dynamics (55 papers). S. P. Owocki collaborates with scholars based in United States, Germany and United Kingdom. S. P. Owocki's co-authors include R. H. D. Townsend, Asif ud‐Doula, Steven R. Cranmer, David H. Cohen, G. B. Rybicki, J. O. Sundqvist, K. G. Gayley, J. Puls, J. Castor and Luc Dessart and has published in prestigious journals such as The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society and Astronomy and Astrophysics.

In The Last Decade

S. P. Owocki

189 papers receiving 6.4k 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.

Time-dependent models of radiatively driven stellar winds. I - Nonlinear evolution of instabilities for a pure absorption model

1988 405 citations S. P. Owocki, G. B. Rybicki et al. The Astrophysical Journal profile →

Peers

Countries citing papers authored by S. P. Owocki

Since Specialization

Citations

This map shows the geographic impact of S. P. Owocki'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 S. P. Owocki with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites S. P. Owocki more than expected).

Fields of papers citing papers by S. P. Owocki

Since Specialization

Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by S. P. Owocki. 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 S. P. Owocki. The network helps show where S. P. Owocki may publish in the future.

Co-authorship network of co-authors of S. P. Owocki

This figure shows the co-authorship network connecting the top 25 collaborators of S. P. Owocki. A scholar is included among the top collaborators of S. P. Owocki 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 S. P. Owocki. S. P. Owocki 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	Efficiency of viscous angular momentum transport in dissipating Be binaries 2025 ·Astrophysics and Space Science ·(unknown), C. E. Jones, K. G. Gayley, A. Granada, S. P. Owocki, (unknown), (unknown), Atsuo T. Okazaki, Asif ud‐Doula, Jiřı́ Krtička, A. C. Carciofi, J. J. Drake	0
2	3D MHD models of the centrifugal magnetosphere from a massive star with an oblique dipole field 2023 ·Monthly Notices of the Royal Astronomical Society ·Asif ud‐Doula, S. P. Owocki, Christopher M. P. Russell, Marc Gagné, (unknown)	7
3	Understanding structure in line-driven stellar winds using ultraviolet spectropolarimetry in the time domain 2022 ·Astrophysics and Space Science ·K. G. Gayley, J. S. Vink, Asif ud‐Doula, Alexandre David-Uraz, Richard Ignace, R. K. Prinja, Nicole St‐Louis, Sylvia Ekström, Yaël Nazé, T. Shenar, Paul A. Scowen, (unknown), S. P. Owocki, J. O. Sundqvist, (unknown), (unknown)	4
4	2D wind clumping in hot, massive stars from hydrodynamical line-driven instability simulations using a pseudo-planar approach 2018 ·Springer Link (Chiba Institute of Technology) ·J. O. Sundqvist, S. P. Owocki, J. Puls	66
5	ETA CARINAE’S THERMAL X-RAY TAIL MEASURED WITH XMM-NEWTON AND NuSTAR 2016 ·The Astrophysical Journal ·Kenji Hamaguchi, M. F. Corcoran, T. R. Gull, H. Takahashi, Brian W. Grefenstette, Takayuki Yuasa, M. Stuhlinger, Christopher M. P. Russell, A. F. J. Moffat, (unknown), Thomas Madura, Noel D. Richardson, J. H. Groh, J. M. Pittard, S. P. Owocki	9
6	A multi-wavelength view of NGC 1624-2 2016 ·Proceedings of the International Astronomical Union ·Alexandre David-Uraz, V. Pétit, (unknown), (unknown), S. P. Owocki, A. W. Fullerton, N. R. Walborn, David H. Cohen	1
7	V444 Cygni X-ray and polarimetric variability: radiative and coriolis forces shape the wind collision region 2015 ·White Rose Research Online (University of Leeds, The University of Sheffield, University of York) ·(unknown), Yaël Nazé, Jennifer L. Hoffman, Christopher M. P. Russell, M. De Becker, M. F. Corcoran, James W. Davidson, Hilding R. Neilson, S. P. Owocki, J. M. Pittard, A. M. T. Pollock	23
8	eta Carinae Emerging from the X-ray Minimum 2014 ·ATel ·M. F. Corcoran, (unknown), Kenji Hamaguchi, T. Gull, Thomas Madura, M. Teodoro, A. F. J. Moffat, Noel D. Richardson, C. T. Russell, (unknown), S. P. Owocki	1
9	An X-Ray Survey of Colliding Wind Binaries 2012 ·ASPC ·Marc Gagné, (unknown), (unknown), (unknown), David H. Cohen, S. P. Owocki	4
10	Continuum‐Driven Winds from Super‐Eddington Stars: A Tale of Two Limits 2008 ·AIP conference proceedings ·Allard Jan van Marle, S. P. Owocki, Nir J. Shaviv	4
11	Active OB-Stars : laboratories for stellar and circumstellar physics : proceedings of a confernece held at Hokkai-Gakuen University, Sapporo, Japan, August 29- September 2, 2005 2007 ·Astronomical Society of the Pacific eBooks ·S. Štefl, S. P. Owocki, (unknown)	1
12	Inferring hot-star-wind acceleration from Line Profile Variability 2005 ·Springer Link (Chiba Institute of Technology) ·Luc Dessart, S. P. Owocki	15
13	On multicomponent effects in stellar winds of stars at extremely\nlow metallicity 2003 ·Springer Link (Chiba Institute of Technology) ·Jiřı́ Krtička, S. P. Owocki, J. Kubát, Ross Galloway, J. C. Brown	13
14	Radiatively Driven Stellar Winds from Hot Stars 2000 ·S. P. Owocki	3
15	Spectral Diagnostics of Blue Stars with Winds 1998 ·ASPC ·(unknown), R. P. Kudritzki, (unknown), A. Alonso‐Herrero, S. P. Owocki, James K. McCarthy	2
16	ThePhysics of Stellar Winds Near the Eddington Limit 1997 ·ASPC ·S. P. Owocki, K. G. Gayley	1
17	Radiation Driven Winds of Hot Stars - some Remarks on Stationary Models and Spectrum Synthesis in Time-Dependent Simulations. (Ludwig Biermann Award Lecture 1992) 1993 ·(unknown), A. W. A. Pauldrach, R. P. Kudritzki, S. P. Owocki, F. Najarro	1
18	Can Nonstationary Velocity Plateaus Account for Slowly Moving Discrete Absorption Components? (Contributed Poster) 1992 ·ASPC ·A. W. Fullerton, S. P. Owocki	2
19	Instabilities in Line-Driven Stellar Winds 1983 ·Bulletin of the American Astronomical Society ·G. B. Rybicki, S. P. Owocki	1
20	The Ionization State of the Solar Wind 1981 ·Bulletin of the American Astronomical Society ·S. P. Owocki	5

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