LabCompass

D. Milisavljević

Physics and Astronomy · Purdue University West Lafayette

Established · publishing since 1999Rising activity

Publications

418

Citations

7,844

Est. group size

~7

Recurring co-author estimate

Active years

28

Publishing since 1999

Research summary
AI-generated

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.

Core-collapse supernovae and their progenitor starsSupernova remnants and explosion mechanismsCircumstellar material and mass-loss history of dying starsMulti-wavelength follow-up (X-ray, radio, infrared) of stellar explosionsFast and unusual optical transients

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

Publication cadence
Publications per year over the last 10 years — averaging 20.8/year recently
2017: 17 publications172018: 14 publications182019: 28 publications192020: 21 publications202021: 20 publications212022: 15 publications222023: 29 publications29232024: 28 publications242025: 28 publications252026: 4 publications26
Recent publications
Publishes in
  • 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
Similar researchers
By research-topic overlap

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.

Claim or correct this profile