论文标题
WHTZ 1：高激发行星星云不是来自失控的星星HD 185806的气态茧
WHTZ 1: A high excitation Planetary Nebula not a gaseous cocoon from runaway star HD 185806
论文作者
论文摘要
我们提供了证据表明，阳离子茧和弓震发射星云是预测的，最近报道是从9级“失控”星HD 185806衍生出来的是先前发现但晦涩的行星星云WHTZ 1（RA 7）。它在其几何中心有一个Gaia Dr3 G〜16蓝色电离星。我们提出图像，光谱，其他数据和参数，以支持这种发射源是高激发的行星星云，而不是恒星的风力弓冲击。
We present evidence that the nebular cocoon and bow-shock emission nebula putatively and recently reported as deriving from the 9th magnitude "runaway" star HD 185806 is the previously discovered but obscure planetary nebula WHTZ 1 (Ra 7). It has a Gaia DR3 G~16 blue ionizing star at its geometric centre. We present imagery, spectroscopy, other data and arguments to support that this emission source is a high excitation Planetary Nebula not a stellar wind bow shock.
