S. T. Megeath

16.2k total citations · 2 hit papers
127 papers, 6.5k citations indexed

About

S. T. Megeath is a scholar working on Astronomy and Astrophysics, Spectroscopy and Atmospheric Science. According to data from OpenAlex, S. T. Megeath has authored 127 papers receiving a total of 6.5k indexed citations (citations by other indexed papers that have themselves been cited), including 120 papers in Astronomy and Astrophysics, 48 papers in Spectroscopy and 16 papers in Atmospheric Science. Recurrent topics in S. T. Megeath's work include Astrophysics and Star Formation Studies (112 papers), Stellar, planetary, and galactic studies (102 papers) and Astro and Planetary Science (44 papers). S. T. Megeath is often cited by papers focused on Astrophysics and Star Formation Studies (112 papers), Stellar, planetary, and galactic studies (102 papers) and Astro and Planetary Science (44 papers). S. T. Megeath collaborates with scholars based in United States, Germany and United Kingdom. S. T. Megeath's 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 and has published in prestigious journals such as Nature, The Astrophysical Journal and Monthly Notices of the Royal Astronomical Society.

In The Last Decade

S. T. Megeath

122 papers receiving 6.2k citations

Hit Papers

A map of the day–night co... 2007 2026 2013 2019 2007 2009 100 200 300 400

Peers — A (Enhanced Table)

Peers by citation overlap · career bar shows stage (early→late) cites · hero ref

Name h Career Trend Papers Cites
S. T. Megeath United States 42 6.3k 1.6k 702 629 175 127 6.5k
John M. Carpenter United States 49 7.0k 1.1× 2.0k 1.3× 478 0.7× 423 0.7× 220 1.3× 166 7.2k
C. J. Clarke United Kingdom 49 7.3k 1.2× 1.6k 1.0× 617 0.9× 241 0.4× 130 0.7× 200 7.5k
Barbara Ercolano Germany 38 5.1k 0.8× 1.1k 0.7× 312 0.4× 324 0.5× 168 1.0× 145 5.3k
Sean M. Andrews United States 43 6.4k 1.0× 2.6k 1.6× 234 0.3× 523 0.8× 270 1.5× 150 6.6k
P. Hennebelle France 45 5.9k 0.9× 1.1k 0.7× 193 0.3× 813 1.3× 388 2.2× 159 6.0k
M. Spaans Netherlands 30 3.3k 0.5× 665 0.4× 204 0.3× 430 0.7× 272 1.6× 87 3.4k
M. H. Heyer United States 37 4.0k 0.6× 1.0k 0.7× 125 0.2× 752 1.2× 193 1.1× 103 4.1k
Pascal Tremblin France 32 2.3k 0.4× 395 0.2× 359 0.5× 627 1.0× 116 0.7× 88 2.6k
Steven V. W. Beckwith United States 22 3.9k 0.6× 870 0.5× 888 1.3× 213 0.3× 264 1.5× 40 4.0k
Shigeru Ida Japan 44 7.0k 1.1× 408 0.3× 542 0.8× 372 0.6× 66 0.4× 153 7.1k

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 of co-authors of S. T. Megeath

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

All Works

20 of 20 papers shown
1.
Girart, J. M., Ian Stephens, Manuel Fernández-López, et al.. (2025). The Protostars in Orion: Characterizing the Properties of Their Magnetized Envelopes. The Astrophysical Journal. 981(1). 30–30. 1 indexed citations
2.
Girart, J. M., Ian Stephens, Philip C. Myers, et al.. (2025). Characterizing Magnetic Properties of Young Protostars in Orion. The Astrophysical Journal. 984(1). 29–29.
3.
Slavicinska, K., Łukasz Tychoniec, E. F. van Dishoeck, et al.. (2025). HDO Ice Detected toward an Isolated Low-mass Protostar with JWST. The Astrophysical Journal Letters. 986(2). L19–L19. 3 indexed citations
4.
Quillen, Alice C., et al.. (2023). HOPS 361-C’s Jet Decelerating and Precessing through NGC 2071 IR. The Astrophysical Journal. 948(1). 39–39.
5.
Pokhrel, Riwaj, S. T. Megeath, Robert Gutermuth, et al.. (2023). Extension of HOPS out to 500 pc (eHOPS). I. Identification and Modeling of Protostars in the Aquila Molecular Clouds*. The Astrophysical Journal Supplement Series. 266(2). 32–32. 19 indexed citations
6.
Tobin, John, Yao-Lun Yang, Merel L. R. van ’t Hoff, et al.. (2022). Disks and Outflows in the Intermediate-mass Star-forming Region NGC 2071 IR. The Astrophysical Journal. 933(2). 178–178. 5 indexed citations
7.
Megeath, S. T., Robert Gutermuth, & Marina Kounkel. (2022). Low Mass Stars as Tracers of Star and Cluster Formation. Publications of the Astronomical Society of the Pacific. 134(1034). 42001–42001. 16 indexed citations
8.
Herczeg, Gregory J., Jeong‐Eun Lee, Doug Johnstone, et al.. (2022). Dissecting the Different Components of the Modest Accretion Bursts of the Very Young Protostar HOPS 373. The Astrophysical Journal. 929(1). 60–60. 18 indexed citations
9.
Habel, Nolan, S. T. Megeath, William J. Fischer, et al.. (2021). An HST Survey of Protostellar Outflow Cavities: Does Feedback Clear Envelopes?. The Astrophysical Journal. 911(2). 153–153. 20 indexed citations
10.
Pokhrel, Riwaj, Robert Gutermuth, Mark R. Krumholz, et al.. (2021). The Single-cloud Star Formation Relation. The Astrophysical Journal Letters. 912(1). L19–L19. 34 indexed citations
11.
Tobin, John, Patrick Sheehan, S. T. Megeath, et al.. (2020). The VLA/ALMA Nascent Disk and Multiplicity (VANDAM) Survey of Orion Protostars. IV. Unveiling the Embedded Intermediate-Mass Protostar and Disk within OMC2-FIR3/HOPS-370. The Astrophysical Journal. 905(2). 162–162. 20 indexed citations
12.
Li, Guang-Xing, F. Wyrowski, K. M. Menten, S. T. Megeath, & Xun Shi. (2015). G-virial: Gravity-based structure analysis of molecular clouds. Springer Link (Chiba Institute of Technology). 12 indexed citations
13.
Bourke, Tyler L., M. R. Hogerheijde, F. F. S. van der Tak, et al.. (2013). Dense molecular cocoons in the massive protocluster W3 IRS5: a test case for models of massive star formation. Springer Link (Chiba Institute of Technology). 7 indexed citations
14.
Hora, Joseph L., S. Bontemps, S. T. Megeath, et al.. (2007). A Spitzer Legacy Survey of the Cygnus-X Complex. 40184. 2 indexed citations
15.
Alam, Shadab, S. T. Megeath, Robert Gutermuth, et al.. (2006). The Structure and Evolution of Young Stellar Clusters. 361. 7 indexed citations
16.
Megeath, S. T., Kevin Flaherty, Joseph L. Hora, et al.. (2005). A Spitzer/IRAC Survey of the Orion Molecular Clouds. 5 indexed citations
17.
Fazio, G. G. & S. T. Megeath. (2004). An IRAC Survey of the L1630 and L1641 (Orion) Molecular Clouds. 43. 1 indexed citations
18.
Megeath, S. T., et al.. (1999). The Detection of Outflows in the Infrared-quiet Molecular Core NGC 6334/I(North). The Astrophysical Journal. 526(2). L113–L116. 20 indexed citations
19.
Megeath, S. T., et al.. (1998). A SURVEY FOR DENSE CORES AND YOUNG STELLAR CLUSTERS IN THE W 3 GIANT MOLECULAR CLOUD. 336(3). 991–1006. 1 indexed citations
20.
Megeath, S. T., et al.. (1998). Star formation toward the "quiescent" core NGC 6334 I(N).. Msngr. 93. 36–38. 1 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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