학술논문

Orbital Period Changes in WZ Sagittae
Document Type
Working Paper
Source
Subject
Astrophysics - Solar and Stellar Astrophysics
Language
Abstract
We report a long-term (1961-2017) study of the eclipse times in the dwarf nova WZ Sagittae, in an effort to learn its rate of orbital-period change. Some wiggles with a time scale of 20-50 years are apparent, and a connection with the 23-year interval between dwarf-nova eruptions is possible. These back-and-forth wiggles dominate the O-C diagram, and prevent a secure measurement of the steady rate of orbital-period change. The line, it is drawn, the curse, it is cast. The slow one now will later be fast... For the times, they are a-changin'. - Dylan (1963)
Comment: PDF, 17 pages, 1 table, 5 figures; submitted, PASP; more info at http://cbastro.org/