T. Peters

1.8k total citations · 1 hit paper
16 papers, 686 citations indexed

About

T. Peters is a scholar working on Astronomy and Astrophysics, Spectroscopy and Nuclear and High Energy Physics. According to data from OpenAlex, T. Peters has authored 16 papers receiving a total of 686 indexed citations (citations by other indexed papers that have themselves been cited), including 16 papers in Astronomy and Astrophysics, 5 papers in Spectroscopy and 2 papers in Nuclear and High Energy Physics. Recurrent topics in T. Peters's work include Astrophysics and Star Formation Studies (15 papers), Stellar, planetary, and galactic studies (11 papers) and Molecular Spectroscopy and Structure (5 papers). T. Peters is often cited by papers focused on Astrophysics and Star Formation Studies (15 papers), Stellar, planetary, and galactic studies (11 papers) and Molecular Spectroscopy and Structure (5 papers). T. Peters collaborates with scholars based in Germany, United Kingdom and United States. T. Peters's co-authors include Ralf S. Klessen, Philipp Girichidis, Richard Wünsch, Thorsten Naab, Stefanie Walch, Simon C. O. Glover, Paul C. Clark, Andrea Gatto, Christian Baczynski and Dominik Derigs and has published in prestigious journals such as Monthly Notices of the Royal Astronomical Society, Astronomy and Astrophysics and The Astrophysical Journal Letters.

In The Last Decade

T. Peters

16 papers receiving 644 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 SILCC (SImulating the LifeCycle of molecular Clouds) project – I. Chemical evolution of the supernova-driven ISM

2015 269 citations Stefanie Walch, Philipp Girichidis et al. Monthly Notices of the Royal Astronomical Society profile →

Peers

T. Peters

SPECT

NHEP

AMPO

N. Vaytet United Kingdom

Kazunari Iwasaki Japan

Christian Baczynski Germany

Anne‐Katharina Jappsen Germany

Andrea Gatto Germany

Pak Shing Li United States

Sam Geen Germany

A. C. Raga Mexico

J. D. Soler Germany

Robin G. Treß Germany

N. Vaytet United Kingdom

T. Peters

641 ×1.0

79 ×0.8

102 ×1.2

SPECT

62 ×0.7

NHEP

48 ×0.9

AMPO

Citations per year, relative to T. Peters T. Peters (= 1×) peers N. Vaytet

Countries citing papers authored by T. Peters

Since Specialization

Citations

This map shows the geographic impact of T. Peters'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 T. Peters with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites T. Peters more than expected).

Fields of papers citing papers by T. Peters

Since Specialization

Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of T. Peters

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

All Works

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16 of 16 papers shown

Beltrán, M. T., V. M. Rivilla, R. Cesaroni, et al.. (2022). The sharp ALMA view of infall and outflow in the massive protocluster G31.41+0.31. Astronomy and Astrophysics. 659. A81–A81. 13 indexed citations

Olguin, Fernando A., M. G. Hoare, K. Johnston, et al.. (2020). Multiwavelength modelling of the circumstellar environment of the massive protostar AFGL 2591 VLA 3. Monthly Notices of the Royal Astronomical Society. 498(4). 4721–4744. 6 indexed citations

Klaassen, Pamela, K. Johnston, J. S. Urquhart, et al.. (2018). The evolution of young HII regions - I. Continuum emission and internal dynamics. White Rose Research Online (University of Leeds, The University of Sheffield, University of York). 9 indexed citations

Pree, C. G. De, Roberto Galván-Madrid, W. M. Goss, et al.. (2018). Flux Density Variations at 3.6 cm in the Massive Star-forming Region W49A. The Astrophysical Journal Letters. 863(1). L9–L9. 2 indexed citations

Walch, Stefanie, Daniel Seifried, S. D. Clarke, et al.. (2018). Synthetic [C ii] emission maps of a simulated molecular cloud in formation. Monthly Notices of the Royal Astronomical Society. 481(4). 4277–4299. 27 indexed citations

Klaassen, Pamela, K. Johnston, J. S. Urquhart, et al.. (2017). The evolution of young HII regions. Astronomy and Astrophysics. 611. A99–A99. 15 indexed citations

Seifried, Daniel, Stefanie Walch, Philipp Girichidis, et al.. (2017). SILCC-Zoom: the dynamic and chemical evolution of molecular clouds. Monthly Notices of the Royal Astronomical Society. 472(4). 4797–4818. 101 indexed citations

Girichidis, Philipp, Thorsten Naab, Stefanie Walch, et al.. (2016). The impact of magnetic fields on the chemical evolution of the supernova-driven ISM. Monthly Notices of the Royal Astronomical Society. 465(4). 4611–4633. 12 indexed citations

Schmidt, W., et al.. (2016). Mach number study of supersonic turbulence: the properties of the density field. Monthly Notices of the Royal Astronomical Society. 460(4). 4483–4491. 27 indexed citations

10.

Gatto, Andrea, Stefanie Walch, Mordecai‐Mark Mac Low, et al.. (2015). Modelling the supernova-driven ISM in different environments. Monthly Notices of the Royal Astronomical Society. 449(1). 1057–1075. 122 indexed citations

11.

Walch, Stefanie, Philipp Girichidis, Thorsten Naab, et al.. (2015). The SILCC (SImulating the LifeCycle of molecular Clouds) project – I. Chemical evolution of the supernova-driven ISM. Monthly Notices of the Royal Astronomical Society. 454(1). 246–276. 269 indexed citations breakdown →

12.

Low, Mordecai‐Mark Mac, T. Peters, Pamela Klaassen, Martin Schrön, & Ralf S. Klessen. (2014). Massive Stellar Outflows From the Combined Action of Multiple Stellar Jets. AAS. 223. 1 indexed citations

13.

Pree, C. G. De, T. Peters, Mordecai‐Mark Mac Low, et al.. (2014). FLICKERING OF 1.3 cm SOURCES IN SGR B2: TOWARD A SOLUTION TO THE ULTRACOMPACT H II REGION LIFETIME PROBLEM. The Astrophysical Journal Letters. 781(2). L36–L36. 31 indexed citations

14.

Klaassen, Pamela, Roberto Galván-Madrid, T. Peters, Steven N. Longmore, & M. Maercker. (2013). Ionization driven molecular outflow in K3-50A. Astronomy and Astrophysics. 556. A107–A107. 6 indexed citations

15.

Galván-Madrid, Roberto, Hauyu Baobab Liu, Zhi-Yu Zhang, et al.. (2013). MUSCLE W49: A multi-scale continuum and line exploration of the most luminous star formation region in the Milky Way. I. Data and the mass structure of the giant molecular cloud. Zurich Open Repository and Archive (University of Zurich). 35 indexed citations

16.

Peters, T., Robi Banerjee, & Ralf S. Klessen. (2008). Ionization front-driven turbulence in the clumpy interstellar medium. Physica Scripta. T132. 14026–14026. 10 indexed citations

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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