Recently, Ph.D. candidate ZANG Lei and Prof. QIAN Shengbang, from Yunnan Observatories of Chinese Academy of Sciences and their cooperator discovered that the orbital evolution of the supersoft X-ray source WX Cen is dominated by the angular momentum loss (AML). The AML is driven by magnetic wind from the donor secondary and that from the accretion disk alone or together. This work was published in The Astrophysical Journal.

WX Cen is most likely one of the Galactic counterparts of close binary supersoft X-ray sources (CBSS) as a member of the V Sagittae class, where mass is transferred from a donor secondary to a massive white dwarf primary via an accretion disk.

To further study their mass exchange and the orbital evolution, the researchers analyzed the orbital period variation of WX Cen in detail, by using the continuous the Transiting Exoplanet Survey Satellite (TESS) light curves and the photometric observations collected by American Association of Variable Star Observers (AAVSO) database. The result implies that the orbital period is continuously decreasing.

Moreover, based on the results of previous research, the researchers estimated that the mass of the donor secondary is about 0.6 solar mass, when the white dwarf mass is about 0.9 solar mass.

By considering a conservative mass transfer from the donor secondary to the white dwarf, the orbital period of WX Cen should be increasing, which is opposite to the observed continuous decrease. Therefore, the decrease in the period can be plausibly explained as the result of AML caused by magnetic wind from the secondary and that from the accretion disk alone or together.

If the Alfvén radius of the secondary gets smaller than 20 solar radius, the mass-loss rate required to reduce the orbital period will be too high to be supported by stellar wind loss alone. And the Alfvén radius of the accretion disk is more than 5.5 solar radius.

Contact:
ZANG Lei
Yunnan Observatories, CAS
Email: zanglei@ynao.ac.cn