Radio studies of novae: A current status report and highlights of new results

Nirupam Roy, Laura Chomiuk, Jennifer L. Sokoloski, Jennifer Weston, Michael P. Rupen, Traci Johnson, Miriam I. Krauss, Thomas Nelson, Koji Mukai, Amy Mioduszewski, Michael F. Bode, Stewart P.S. Eyres, Tim J. O'Brien

Research output: Contribution to journalArticlepeer-review


Novae, which are the sudden visual brightening triggered by runaway thermonuclear burning on the surface of an accreting white dwarf, are fairly common and bright events. Despite their astronomical significance as nearby laboratories for the study of nuclear burning and accretion phenomena, many aspects of these common stellar explosions are observationally not well-constrained and remain poorly understood. Radio observations, modeling and interpretation can potentially play a crucial role in addressing some of these puzzling issues. In this review on radio studies of novae, we focus on the possibility of testing and improving the nova models with radio observations, and present a current status report on the progress in both the observational front and theoretical developments. We specifically address the issues of accurate estimation of ejecta mass, multi-phase and complex ejection phenomena, and the effect of a dense environment around novae. With highlights of new observational results, we illustrate how radio observations can shed light on some of these longstanding puzzles.

Original languageEnglish
Pages (from-to)293-310
Number of pages18
JournalBulletin of the Astronomical Society of India
Issue number3
Publication statusPublished - 1 Dec 2012


  • Novae, Cataclysmic variables
  • Radio continuum: Stars
  • White dwarfs


Dive into the research topics of 'Radio studies of novae: A current status report and highlights of new results'. Together they form a unique fingerprint.

Cite this