We present the result of additional high-speed photometric observation of HD 137949. The Johnson-B photometric data were obtained on five nights between 2013 July 31, and August 19, using 0.5-m optical telescope of the South African Astronomical Observatory (SAAO). Frequency analysis of our nightly data sets as well as combination of all data sets reveal no new oscillation besides the well-known principal frequency of oscillation ($\nu =2.01478$mHz). However, frequency analysis of a combination of our current data set and the old data set acquired few months earlier reveals that the principal frequency of oscillation has remained stable at ${\nu }_1=2.014781\pm 0.000003$mHz for over three decades. Two new secondary frequencies were also detected on either side of the principal frequency at ${\nu }_2=2.016787\pm 0.000006$mHz and ${\nu }_3=2.012628\pm 0.000009$mHz. We discuss all possible implications as regards this recent excitation of ${\nu }_2$and ${\nu }_3$vis-a-vis the mystery surrounding the oscillations and real rotation period of HD 137949.

我们介绍了HD 137949的额外高速光度学观测结果。Johnson- B光度数据是在2013年7月31日至8月19日的五个晚上使用南非天文台（SAAO）的0.5米光学望远镜获得的。 。我们对夜间数据集的频率分析以及所有数据集的组合显示，除了众所周知的主要振荡频率（$\nu =2.01478$mHz）。但是，对我们的当前数据集和几个月前获取的旧数据集进行的频率分析显示，振荡的主频率保持稳定在${\nu }_{\mathrm{1个}}=2.014781\pm 0.000003$mHz超过三十年。在主频率的两侧还检测到两个新的次级频率${\nu }_2=2.016787\pm 0.000006$兆赫兹和 ${\nu }_3=2.012628\pm 0.000009$兆赫 我们讨论了有关这方面最近的兴奋的所有可能的含义。${\nu }_2$和 ${\nu }_3$相对于HD 137949的振荡和实际旋转周期的奥秘。