Dina K. Prialnik

brightness. i.e. T Aurigae (+3.8) was a brighter nova than HR Lyrae (+6.5) Prialnik, Dina. "Novae", pp. 1846-56, in Paul Murdin, ed. Encyclopedia of Astronomy

1016/j.icarus.2021.114574. 114574. Grundy, William M. (1 January 2020). Prialnik, Dina; Barucci, M. Antonietta; Young, Leslie A. (eds.). The Trans-Neptunian

vol. 3, Cambridge University Press, p. 27, ISBN 978-0-521-57244-6 Prialnik, Dina (2000), An Introduction to the Theory of Stellar Structure and Evolution

and Astrophysics. 246 (2): L77 – L80. Bibcode:1991A&A...246L..77W. Prialnik, Dina; Bar-Nun, Akiva (1992). "Crystallization of amorphous ice as the cause

structure, and evolution (2nd ed.). Springer-Verlag. ISBN 0-387-20089-4. Prialnik, Dina (2000). An Introduction to the Theory of Stellar Structure and Evolution