Hubert Klahr

12.6k total citations · 3 hit papers
115 papers, 6.8k citations indexed

About

Hubert Klahr is a scholar working on Astronomy and Astrophysics, Spectroscopy and Fluid Flow and Transfer Processes. According to data from OpenAlex, Hubert Klahr has authored 115 papers receiving a total of 6.8k indexed citations (citations by other indexed papers that have themselves been cited), including 112 papers in Astronomy and Astrophysics, 17 papers in Spectroscopy and 5 papers in Fluid Flow and Transfer Processes. Recurrent topics in Hubert Klahr's work include Astrophysics and Star Formation Studies (107 papers), Stellar, planetary, and galactic studies (88 papers) and Astro and Planetary Science (87 papers). Hubert Klahr is often cited by papers focused on Astrophysics and Star Formation Studies (107 papers), Stellar, planetary, and galactic studies (88 papers) and Astro and Planetary Science (87 papers). Hubert Klahr collaborates with scholars based in Germany, United States and Switzerland. Hubert Klahr's co-authors include Thomas Henning, Anders Johansen, Chris W. Ormel, Th. Henning, C. Mordasini, Y. Alibert, T. Birnstiel, Peter Bodenheimer, Barbara Ercolano and Wladimir Lyra and has published in prestigious journals such as Nature, SHILAP Revista de lepidopterología and The Astrophysical Journal.

In The Last Decade

Hubert Klahr

114 papers receiving 6.4k citations

Hit Papers

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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.

Rapid planetesimal formation in turbulent circumstellar disks

2007 750 citations Anders Johansen, Hubert Klahr et al. profile →
A simple model for the evolution of the dust population in protoplanetary disks

2012 502 citations T. Birnstiel, Hubert Klahr et al. Astronomy and Astrophysics profile →
The effect of gas drag on the growth of protoplanets

2010 374 citations Hubert Klahr et al. Astronomy and Astrophysics profile →

Peers

Countries citing papers authored by Hubert Klahr

Since Specialization

Citations

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

Fields of papers citing papers by Hubert Klahr

Since Specialization

Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by Hubert Klahr. 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 Hubert Klahr. The network helps show where Hubert Klahr may publish in the future.

Co-authorship network of co-authors of Hubert Klahr

This figure shows the co-authorship network connecting the top 25 collaborators of Hubert Klahr. A scholar is included among the top collaborators of Hubert Klahr 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 Hubert Klahr. Hubert Klahr is excluded from the visualization to improve readability, since they are connected to all nodes in the network.

All Works

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20 of 20 papers shown

#	Work	Indexed citations
1	TriPoD: Tri-Population size distributions for Dust evolution 2024 ·Astronomy and Astrophysics ·(unknown), T. Birnstiel, Hubert Klahr	3
2	Vertical shear instability with dust evolution and consistent cooling times 2024 ·Astronomy and Astrophysics ·(unknown), T. Birnstiel, Hubert Klahr	4
3	Spiral excitation in protoplanetary disks through gap-edge illumination 2024 ·Astronomy and Astrophysics ·(unknown), (unknown), Hubert Klahr	5
4	High-resolution Study of Planetesimal Formation by Gravitational Collapse of Pebble Clouds 2023 ·The Astrophysical Journal ·(unknown), Hubert Klahr	7
5	Vertical shear instability in two-moment radiation-hydrodynamical simulations of irradiated protoplanetary disks 2023 ·Astronomy and Astrophysics ·(unknown), Mario Flock, Hubert Klahr	11
6	Dust Coagulation Reconciles Protoplanetary Disk Observations with the Vertical Shear Instability. I. Dust Coagulation and the VSI Dead Zone 2023 ·The Astrophysical Journal ·(unknown), T. Birnstiel, Hubert Klahr	17
7	Three-temperature radiation hydrodynamics with PLUTO 2023 ·Astronomy and Astrophysics ·(unknown), (unknown), Hubert Klahr	16
8	Resilience of Planetesimal Formation in Weakly Reinforced Pressure Bumps 2022 ·The Astrophysical Journal ·Daniel Carrera, Andrew Thomas, Jacob B. Simon, (unknown), Katherine A. Kretke, Hubert Klahr	19
9	Effect of pebble flux-regulated planetesimal formation on giant planet formation 2020 ·Springer Link (Chiba Institute of Technology) ·(unknown), Hubert Klahr, C. Mordasini, Alexandre Emsenhuber, Christian Lenz	17
10	Global axisymmetric simulations of photoevaporation and magnetically driven protoplanetary disk winds 2019 ·Springer Link (Chiba Institute of Technology) ·(unknown), Hubert Klahr, Christian Fendt, C. P. Dullemond	19
11	Linking planetesimal and dust content in protoplanetary disks via a local toy model 2019 ·Springer Link (Chiba Institute of Technology) ·(unknown), Christian Lenz, Hubert Klahr	18
12	Gaps, rings, and non-axisymmetric structures in protoplanetary disks: Emission from large grains 2016 ·Springer Link (Chiba Institute of Technology) ·(unknown), Mario Flock, S. Wolf, Natalia Dzyurkevich, S. Fromang, Th. Henning, Hubert Klahr, H. Méheut	51
13	Planet-induced disk structures: A comparison between (sub)mm and infrared radiation 2014 ·Springer Link (Chiba Institute of Technology) ·(unknown), S. Wolf, Ana Uribe, Hubert Klahr	8
14	A survey of young, nearby, and dusty stars conducted to understand the formation of wide-orbit giant planets - VLT/NaCo adaptive optics thermal and angular differential imaging 2013 ·Max Planck Institute for Plasma Physics ·Julien Rameau, G. Chauvin, A.‐M. Lagrange, Hubert Klahr, M. Bonnefoy, C. Mordasini, M. Bonavita, S. Desidera, Christophe Dumas, J. H. Girard	31
15	On the stability of radiation-pressure-dominated cavities 2012 ·Springer Link (Chiba Institute of Technology) ·R. Kuiper, Hubert Klahr, H. Beuther, Th. Henning	39
16	High-order Godunov schemes for global 3D MHD simulations of accretion disks. I. Testing the linear growth of the magneto-rotational instability 2010 ·Max Planck Institute for Plasma Physics ·Mario Flock, Natalia Dzyurkevich, Hubert Klahr, A. Mignone	24
17	Fast and accurate frequency-dependent radiation transport for hydrodynamics simulations in massive star formation 2010 ·Springer Link (Chiba Institute of Technology) ·R. Kuiper, Hubert Klahr, C. P. Dullemond, W. Kley, Thomas Henning	84
18	A coagulation-fragmentation model for the turbulent growth and destruction of preplanetesimals 2008 ·Springer Link (Chiba Institute of Technology) ·Anders Johansen, F. Brauer, C. P. Dullemond, Hubert Klahr, Thomas Henning	24
19	A three phase model for planet formation - the formation of a planet in the eye of a hurricane 2003 ·ESASP ·Hubert Klahr, Peter Bodenheimer	2
20	Turbulence in Accretion Discs. The Global Baroclinic Instability 2001 ·Hubert Klahr, Peter Bodenheimer	1

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.

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