Nova
Tampilan
![](http://178.128.105.246/cars-http-upload.wikimedia.org/wikipedia/commons/5/5d/Making_a_Nova.jpg)
Nova adalah ledakan nuklir kataklismik yang disebabkan oleh akresi hidrogen ke permukaan sebuah katai putih. Fisis ledakan ini berbeda dengan yang terjadi pada supernova dan nova merah cerlang.
Bacaan lanjutan
[sunting | sunting sumber]- Payne-Gaposchkin, C. (1957). The Galactic Novae. North Holland Publishing Co.
- Hernanz, M.; Josè, J. (2002). Classical Nova Explosions. American Institute of Physics.
- Bode, M.F.; Evans, E. (2008). Classical Novae. Cambridge University Press.
Pranala luar
[sunting | sunting sumber]![](http://178.128.105.246/cars-http-upload.wikimedia.org/wikipedia/commons/thumb/4/4a/Commons-logo.svg/30px-Commons-logo.svg.png)
Wikimedia Commons memiliki media mengenai Nova.
- Schaefer (2009). "Comprehensive Photometric Histories of All Known Galactic Recurrent Novae". The Astrophysical Journal Supplement Series. 187: 275–373. arXiv:0912.4426
. Bibcode:2010ApJS..187..275S. doi:10.1088/0067-0049/187/2/275.
- Shafter; et al. (2011). "A Spectroscopic and Photometric Survey of Novae in M31". The Astrophysical Journal. 734: 12. arXiv:1104.0222
. Bibcode:2011ApJ...734...12S. doi:10.1088/0004-637X/734/1/12.
- General Catalog of Variable Stars, Sternberg Astronomical Institute, Moscow
- AAVSO Variable Star of the Month. Novae: May 2001 Diarsipkan 2007-05-19 di Wayback Machine.
- Extragalactic Novae