Optical light curves of RS Oph (2006) and hydrogen burning turnoff
| dc.creator | Hachisu, Izumi | |
| dc.creator | Kato, Mariko | |
| dc.creator | Kiyota, Seiichiro | |
| dc.creator | Kubotera, Katsuaki | |
| dc.creator | Maehara, Hiroyuki | |
| dc.creator | Nakajima, Kazuhiro | |
| dc.creator | Ishii, Yuko | |
| dc.creator | Kamada, Mari | |
| dc.creator | Mizoguchi, Sahori | |
| dc.creator | Nishiyama, Shinji | |
| dc.creator | Sumitomo, Naoko | |
| dc.creator | Tanaka, Ken'ichi | |
| dc.creator | Yamanaka, Masayuki | |
| dc.creator | Sadakane, Kozo | |
| dc.date | 2008-07-08 | |
| dc.date.accessioned | 2026-07-07T09:49:05Z | |
| dc.date.available | 2026-07-07T09:49:05Z | |
| dc.description | We report a coordinated multi-band photometry of the RS Oph 2006 outburst and highlight the emission line free y-band photometry that shows a mid-plateau phase at y ~ 10.2 mag from day 40 to day 75 after the discovery followed by a sharp drop of the final decline. Such mid-plateau phases are observed in other two recurrent novae, U Sco and CI Aql, and are interpreted as a bright disk irradiated by the white dwarf. We have calculated theoretical light curves based on the optically thick wind theory and have reproduced the early decline, mid-plateau phase, and final decline. The final decline is identified with the end of steady hydrogen shell-burning, which turned out at about day 80. This turnoff date is consistent with the end of a supersoft X-ray phase observed with Swift. Our model suggests a white dwarf mass of 1.35 \pm 0.01 M_\sun, which indicates that RS Oph is a progenitor of Type Ia supernovae. We strongly recommend the y-filter observation of novae to detect both the presence of a disk and the hydrogen burning turnoff. Observational data of y magnitudes are provided here together with other multi-wavelength light curve data. | |
| dc.description | 6 pages, 1 figures, Proceeding of "RS Ophiuchi (2006)" conference held at Keele, 12-14 June 2007 | |
| dc.identifier | https://arxiv.org/abs/0807.1240 | |
| dc.identifier | http://arxiv.org/abs/0807.1240 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/164451 | |
| dc.subject | Astrophysics | |
| dc.title | Optical light curves of RS Oph (2006) and hydrogen burning turnoff | |
| dc.type | text |