Speaker
Dr
Jingzhi Yan
(Purple Mountain Obs.)
Description
We present the results of the long-term near infrared (NIR) photometric observations on IGR~J16318-4848. Two period of 26.7 days and 79.7 days are found in the Swift/BAT light curve. A similar 80-day period is found from the JHK light curve of IGR~J16318. The 26.7-day period is interpreted as the orbital period of the system and the neutron star moves in the dense circumstellar disk of the supergiant star. The same 80-day period found both in the Swift/BAT and the JHK light curves might be due to the precession of the circumstellar disk, which caused by the tidal motion of the neutron star.
Primary author
Dr
Jingzhi Yan
(Purple Mountain Obs.)