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| Paper: |
Newly Arising Problems in Research on SU UMa-type Dwarf Novae from VSNet Collaborations |
| Volume: |
362, The Seventh Pacific Rim Conference on Stellar Astrophysics |
| Page: |
195 |
| Authors: |
Nogami, D. |
| Abstract: |
Our research on variable objects based on the VSNET collaborations has achieved much progress in understanding the nature of many kinds of phenomena. Many problems have also appeared, however. Among them, we here review three newly arising problems in research on SU UMa-type dwarf novae: 1) how do EI Psc and V485 Cen evolve as cataclysmic variables?, 2) is the early superhump a particular phenomenon for WZ Sge-type dwarf novae?, and 3) what parameters determine variations of the superhump period? |
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