D. Milisavljević
Physics and Astronomy · Purdue University West Lafayette
Publications
418
Citations
7,844
Est. group size
~7
Recurring co-author estimate
Active years
28
Publishing since 1999
D. Milisavljević studies exploding stars (supernovae) and their aftermath, including supernova remnants, using observations across radio, optical, X-ray, and infrared light. Much of the work focuses on tracking what happens to massive stars before and after they explode, such as the material they shed and how the explosion debris interacts with surrounding gas. This research helps explain how different types of stellar explosions occur and how they seed space with material for future stars and planets.
Publication output has been steady to growing over the last decade, rising from roughly 15-20 papers per year around 2017-2022 to about 28-29 papers per year in 2023-2025.
Generated by claude-sonnet-5 from public bibliographic data · Jul 20, 2026
- Data-driven core-collapse supernova multilateration with first neutrino events
Physical review. D/Physical review. D. · 2026
- A 14-yr-old Mystery: The Peculiar Case of the Engine-driven SN 2012ap
The Astrophysical Journal Letters · 2026
- The Progenitor of the Type II-Plateau SN 2025pht in NGC 1637: The Dustiest, Most Luminous Red Supergiant So Far?
The Astrophysical Journal · 2026
- Dinosaur in a Haystack: X-Ray View of the Entrails of SN 2023ixf and the Radio Afterglow of Its Interaction with the Medium Spawned by the Progenitor Star (Paper I)*
The Astrophysical Journal · 2025
- Filamentary ejecta network in Cassiopeia A reveals fingerprints of the supernova explosion mechanism
Astronomy and Astrophysics · 2025
- The Most Luminous Known Fast Blue Optical Transient AT 2024wpp: Unprecedented Evolution and Properties in the X-Rays and Radio
The Astrophysical Journal Letters · 2025
- The Immediate, Exemplary, and Fleeting Echelle Spectroscopy of SN 2023ixf: Monitoring Acceleration of Slow Progenitor Circumstellar Material Driven by Shock Interaction
The Astrophysical Journal · 2025
- Two Decades of Dust Evolution in SN 2005af through JWST, Spitzer, and Chemical Modeling
The Astrophysical Journal · 2025
- The First Radio View of a Type Ibn Supernova in SN 2023fyq: Understanding the Mass-loss History in the Last Decade before the Explosion
The Astrophysical Journal Letters · 2025
- Hubble Space Telescope Deep Upper Limits Rule out a Surviving Massive Binary Companion to the Type Ic Supernova 2012fh
The Astrophysical Journal · 2025
- Core-collapse supernovae
Elsevier eBooks · 2025
- Core-collapse supernovae
arXiv (Cornell University) · 2025
- The Most Luminous Known Fast Blue Optical Transient AT 2024wpp: Unprecedented Evolution and Properties in the Ultraviolet to the Near-Infrared
arXiv (Cornell University) · 2025
- The Most Luminous Known Fast Blue Optical Transient AT 2024wpp: Unprecedented Evolution and Properties in the X-rays and Radio
arXiv (Cornell University) · 2025
- HST Deep Upper Limits Rule Out a Surviving Massive Binary Companion to the Type Ic Supernova 2012fh
arXiv (Cornell University) · 2025
- arXiv (Cornell University)×50
- The Astrophysical Journal×40
- Monthly Notices of the Royal Astronomical Society×18
- The Astrophysical Journal Letters×17
- VizieR Online Data Catalog×8
- Abigail Polin
Physics and Astronomy · Purdue University West Lafayette
- F. Aros
Physics and Astronomy · Indiana University
- Dimitrios Giannios
Physics and Astronomy · Purdue University West Lafayette
- Danny Milisavljevic
Physics and Astronomy · Purdue University West Lafayette
- G. H. Sembroski
Physics and Astronomy · Purdue University West Lafayette
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 20, 2026.
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