Nova
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.
Selama letusan nova, selubung kaya hidrogen mengembang hingga mencapai ukuran raksasa, disertai percepatan kehilangan massa melalui angin bintang. Ledakan semacam ini telah dimodelkan oleh berbagai peneliti menggunakan kode evolusi tipe Henyey[1]
Bacaan lanjutan
- 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
- 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
| Pembentukan | |
|---|---|
| Nasib | |
| Dalam tata biner | |
| Sifat | |
| Terkait | |
| Internasional | |
|---|---|
| Nasional | |
| Lain-lain | |
 | Artikel bertopik astronomi ini adalah sebuah rintisan. Anda dapat membantu Wikipedia dengan mengembangkannya. |
- ^ Kato, Mariko; Saio, Hideyuki; Hachisu, Izumi (20 Juli 2015). "MULTI-WAVELENGTH LIGHT CURVE MODEL OF THE ONE YEAR RECURRENCE PERIOD NOVA M31N 2008-12a". The Astrophysical Journal. 808 (52): 1–4. doi:10.1088/0004-637x/808/1/52/pdf.
Content Disclaimer
Informasi ini disarikan dari Wikipedia dan disajikan kembali untuk tujuan edukasi. Konten tersedia di bawah lisensi CC BY-SA 3.0. Kami tidak bertanggung jawab atas ketidakakuratan data yang bersumber dari kontribusi publik tersebut.
- The information displayed on this website is sourced in part or in whole from Wikipedia and has been adapted for the purpose of restating it. We strive to provide accurate and relevant information, however:
- There is no guarantee of absolute accuracy. Wikipedia is an open, collaborative project that can be edited by anyone, so information is subject to change.
- It is not intended to constitute professional advice. The content displayed is for informational and educational purposes only. For important decisions (e.g., medical, legal, or financial), please consult a professional.
- Content copyright. Wikipedia is licensed under the Creative Commons Attribution-ShareAlike License (CC BY-SA). This means that content may be reused with appropriate attribution and shared under a similar license.
- Responsible use. Any risk arising from the use of information from this website is entirely the responsibility of the user.