Bibliographic Details
| Title: |
Orbital Period Increase in ES Ceti |
| Authors: |
de Miguel, Enrique, Patterson, Joseph, Kemp, Jonathan, Myers, Gordon, Rea, Robert, Krajci, Thomas, Monard, Berto, Cook, Lewis |
| Publication Year: |
2018 |
| Collection: |
Astrophysics |
| Subject Terms: |
Astrophysics - Solar and Stellar Astrophysics |
| More Details: |
We report a long-term study of the eclipse times in the 10-minute helium binary ES Ceti. The binary period increases rapidly, with P/P-dot = 6.2x10^6 yr. This is consistent with the assumption that gravitational radiation (GR) drives the mass transfer, and appears to be the first dynamical evidence that GR is indeed the driver of evolution in this class of very old cataclysmic variables -- the AM Canum Venaticorum stars.
Comment: PDF, 9 pages, 1 table, 1 figure; accepted, in press, ApJ; more info at http://cbastro.org/ |
| Document Type: |
Working Paper |
| DOI: |
10.3847/1538-4357/aa9ed6 |
| Access URL: |
http://arxiv.org/abs/1801.01049 |
| Accession Number: |
edsarx.1801.01049 |
| Database: |
arXiv |
