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On the induced activity of red dwarfs in close binary systems
| Content Provider | Scilit |
|---|---|
| Author | Ikhsanov, N. R. |
| Copyright Year | 2004 |
| Description | AE Aquarii is a star with unique flaring activity. It is a close binary system, which contains a K3V-K5V red dwarf (secondary) and a magnetized white dwarf rotating with the period of 33 s (primary). It is traditionally classified as a peculiar nova-like star and assigned to the DQ Her subclass of magnetic Cataclysmic Variables (CVs).To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html |
| Related Links | https://www.cambridge.org/core/services/aop-cambridge-core/content/view/F7CF7505954EF274C06CD0A404BE34D0/S1743921304007318a.pdf/div-class-title-on-the-induced-activity-of-red-dwarfs-in-close-binary-systems-div.pdf |
| Ending Page | 684 |
| Page Count | 2 |
| Starting Page | 683 |
| ISSN | 17439213 |
| e-ISSN | 17439221 |
| DOI | 10.1017/s1743921304007318 |
| Journal | Proceedings of the International Astronomical Union |
| Issue Number | IAUS223 |
| Volume Number | 2004 |
| Language | English |
| Publisher | Cambridge University Press (CUP) |
| Publisher Date | 2004-06-01 |
| Access Restriction | Open |
| Subject Keyword | Proceedings of the International Astronomical Union |
| Content Type | Text |
| Resource Type | Article |
| Subject | Astronomy and Astrophysics Space and Planetary Science |