P. M. Lugger
Physics and Astronomy · Indiana University
Publications
148
Citations
2,201
Est. group size
—
Recurring co-author estimate
Active years
49
Publishing since 1978
P. M. Lugger studies dense stellar clusters called globular clusters, focusing on unusual objects within them such as X-ray binaries, cataclysmic variables (compact star pairs that emit bursts of light), neutron stars, and blue straggler stars. The research combines observations from major telescopes, including the Chandra X-ray Observatory, the Hubble Space Telescope, and radio arrays, to identify and characterize these faint and exotic sources.
Publication activity has been steady, with a modest increase in recent years (from around 1-2 per year mid-decade to 3-4 per year most recently).
Generated by claude-opus-4-8 from public bibliographic data · Jul 11, 2026
- Revisiting the Evidence for Double Sequences of Blue Straggler Stars in Globular Clusters
arXiv (Cornell University) · 2026
- Revisiting the Evidence for Double Sequences of Blue Straggler Stars in Globular Clusters
arXiv (Cornell University) · 2026
- Revisiting the Evidence for Double Sequences of Blue Straggler Stars in Globular Clusters
The Astronomical Journal · 2026
- Searching for exotic object companions in the dense core of NGC 362
Astronomy and Astrophysics · 2025
- A Comprehensive Analysis of X-ray Sources in Terzan 5 Using Chandra Observations
arXiv (Cornell University) · 2025
- A Comprehensive Analysis of X-Ray Sources in Terzan 5 Using Chandra Observations
The Astrophysical Journal · 2025
- <i>Chandra</i> and <i>HST</i> studies of the X-ray sources in the globular cluster NGC 362
Monthly Notices of the Royal Astronomical Society · 2024
- Simultaneous <i>Chandra</i> and <i>HST</i> observations of the quiescent neutron star low-mass X-ray binaries in 47 Tucanae
Monthly Notices of the Royal Astronomical Society · 2024
- Chandra and HST studies of the X-ray sources in the Globular Cluster NGC 362
arXiv (Cornell University) · 2024
- Simultaneous Chandra and HST observations of the quiescent neutron-star low-mass X-ray binaries in 47 Tucanae
arXiv (Cornell University) · 2024
- Exotica in the globular cluster M4, studied with <i>Chandra</i>, <i>HST</i>, and the VLA
Monthly Notices of the Royal Astronomical Society · 2023
- Exploration of faint X-ray and radio sources in the massive globular cluster M14: a UV-bright counterpart to Nova Ophiuchus 1938
Monthly Notices of the Royal Astronomical Society · 2023
- Exotica in the Globular Cluster M4, Studied with Chandra, HST, and the VLA
arXiv (Cornell University) · 2023
- Erratum: “Identification of Faint Chandra X-Ray Sources in the Core-collapsed Globular Cluster NGC 6397: Evidence for a Bimodal Cataclysmic Variable Population” (2010, ApJ, 722, 20)
The Astrophysical Journal · 2022
- A deep search for faint <i>Chandra</i> X-ray sources, radio sources, and optical counterparts in NGC 6752
Monthly Notices of the Royal Astronomical Society · 2021
- Monthly Notices of the Royal Astronomical Society×9
- arXiv (Cornell University)×8
- The Astrophysical Journal×2
- Astronomy and Astrophysics×1
- UvA-DARE (University of Amsterdam)×1
This profile was generated automatically from public scholarly data (OpenAlex). Group size and activity levels are estimates derived from co-authorship patterns.
Last updated Jul 11, 2026.
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