H. N. Cohn
Physics and Astronomy · Indiana University
Publications
197
Citations
3,700
Est. group size
—
Recurring co-author estimate
Active years
50
Publishing since 1977
H. N. Cohn studies dense stellar systems called globular clusters, which are tightly packed groups of hundreds of thousands of stars. The research focuses on identifying and characterizing faint objects within these clusters, such as white dwarfs (dead stellar remnants), cataclysmic variables (interacting binary stars), and millisecond pulsars (rapidly spinning neutron stars), often using X-ray observations from the Chandra space telescope.
Publication activity has been steady over the last decade, with a modest increase in recent years (around three to four papers annually since 2023).
Generated by claude-opus-4-8 from public bibliographic data · Jul 11, 2026
- A Search for Helium-Core White Dwarfs in the Globular Cluster 47 Tuc
CSUN ScholarWorks (California State University, Northridge) · 2019
- Identifications of faint<i>Chandra</i>sources in the globular cluster M3
Monthly Notices of the Royal Astronomical Society · 2018
- The Faint CVs and MSPs of the Globular Cluster NGC 6752
Chandra Proposal · 2016
- Monthly Notices of the Royal Astronomical Society×10
- arXiv (Cornell University)×8
- The Astrophysical Journal×2
- Astronomy and Astrophysics×1
- CSUN ScholarWorks (California State University, Northridge)×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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