在色星等图上，处于造父不稳定带的左外侧而温度较高，故简称热造父变星。
On the colour-magnitude diagram they are situated near and more left than the hotter edge of the Cepheid instability stripe, so their temperature is higher than other types of pulsating variables.
在色星等图上，处于造父不稳定带的左外侧而温度较高，故简称热造父变星。
On the colour-magnitude diagram they are situated near and more left than the hotter edge of the Cepheid instability stripe, so their temperature is higher than other types of pulsating variables.
应用推荐