B. J. McNamara

New Mexico State University

Papers

1

Total Citations

60

H-Index

1

About

B. J. McNamara is a stellar astronomer whose work has reshaped our understanding of binary star evolution, particularly through the lens of period changes in Algol-type systems. His landmark 2006 paper, "The Case for Third Bodies as the Cause of Period Changes in Selected Algol Systems," has garnered 60 citations and remains a foundational reference in the field. In this study, McNamara leveraged data from the Robotic Optical Transient Search Experiment (ROTSE-I) and the New Mexico State University 1 m telescope to demonstrate that many long-term orbital period variations in eclipsing binaries are driven by the gravitational influence of a third stellar companion, rather than by mass transfer or magnetic activity alone. This work provided compelling observational evidence for hierarchical triple systems, fundamentally altering how astronomers interpret O–C diagrams. McNamara’s contributions extend to the broader study of variable stars and time-domain astronomy, where his meticulous analysis of archival photometric data has enabled precise measurements of stellar dynamics. His research continues to inform models of binary formation and evolution, making him a key figure in understanding the complex interactions that shape stellar systems.

Research Focus

Key Achievements

1
H-Index
1
Papers
60
Total Citations
60
Avg Citations/Paper
🏆 Most Cited Paper
The Case for Third Bodies as the Cause of Period Changes in Selected Algol Systems
60 citations · 2006
📈 Most Prolific Year: 2006 (1 Papers)
🤝 Key Collaborators: 5
🏛 Institutions: New Mexico State University

Top Papers

  1. 1

Key Collaborators

Contact & Links

Available for collaboration
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