S. T. Megeath

16.2k citations
127 papers · 6.5k indexed · 2 hit papers · h-index 42

S. T. Megeath

122 papers receiving 6.2k citations

Hit Papers

A SPITZER SURVEY OF YOUNG STELLAR CLUSTERS WITHIN ONE KIL...4002007202620132019100200300400

Peers

S. T. Megeath
Comparison fields: 5 of 71
  • Astronomy and Astrophysics 6.3k
  • Instrumentation 702
  • Spectroscopy 1.6k
  • Atmospheric Science 629
  • Fluid Flow and Transfer Processes 138
Replace C. J. Clarke with:
C. J. Clarke United Kingdom
John M. Carpenter United States
Sean M. Andrews United States
Barbara Ercolano Germany
Paolo Padoan United States
M. Spaans Netherlands
P. Hennebelle France
Adam Ginsburg United States
Eduard I. Vorobyov Russia
Christoph Federrath Australia
S. T. Megeath relative to C. J. Clarke United Kingdom C. J. Clarke's profile →
Citations per field
00.5×2.6×
C. J. Clarke · 1×
Citations per year

Countries citing papers authored by S. T. Megeath

Since Specialization
Citations

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

Fields of papers citing papers by S. T. Megeath

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network

The 25 scholars most cited alongside S. T. Megeath, linked wherever they have co-authored with each other. Click a name or a connecting line to browse the papers they share.

Border = papers with S. T. Megeath Line = papers co-authored together S. T. Megeath links everyone, so they are left out of the graph.

All Works

20 of 20 papers shown
#Work
1 20251
2 20250
3 20253
4 20240
5 202319
6 20230
7 20225
8 202218
9 202216
10 202134
11 202120
12 20207
13 202020
14 201748
15 201753
16 201618
17 201512
18 20137
19 199920
20
Star formation toward the "quiescent" core NGC 6334 I(N).
19981

About S. T. Megeath

S. T. Megeath is a scholar working on Astronomy and Astrophysics, Spectroscopy and Instrumentation, having authored 127 papers that have together received 6.5k indexed citations. Recurring topics across this work include Astrophysics and Star Formation Studies (112 papers), Stellar, planetary, and galactic studies (102 papers), Astro and Planetary Science (44 papers), Molecular Spectroscopy and Structure (42 papers), Atmospheric Ozone and Climate (15 papers), Astronomy and Astrophysical Research (9 papers), Spectroscopy and Laser Applications (6 papers) and Astrophysical Phenomena and Observations (6 papers). The work is most often cited by research in Astronomy and Astrophysics (6.3k citations), Instrumentation (702 citations) and Spectroscopy (1.6k citations). S. T. Megeath has collaborated with scholars based in United States, Germany and United Kingdom. Frequent co-authors include Shadab Alam, Robert Gutermuth, G. G. Fazio, Philip C. Myers, James Muzerolle, J. L. Pipher, Lee Hartmann, Nuria Calvet, J. R. Stauffer and Heather A. Knutson. Their work appears in journals such as Nature, The Astrophysical Journal and Monthly Notices of the Royal Astronomical Society.

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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