We report the detection of 21 cm line emission from H I in the planetary nebula NGC 7293 (the Helix Nebula). The observations, made with the Very Large Array, show the presence of a ring of atomic hydrogen that is associated with the outer portion of the ionized nebula. This ring is most probably gas ejected in the asymptotic giant branch phase that has been subsequently photodissociated by radiation from the central star. The H I emission spreads over ~50 km s-1 in radial velocity. The mass in H I is ~0.07 M☉, about 3 times larger than the mass in molecular hydrogen and comparable to the mass in ionized hydrogen.
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机译:我们报告了在行星状星云NGC 7293(螺旋星云)中从H I探测到21厘米线发射的信号。用超大型阵列进行的观测表明存在与离子化星云外部相关的原子氢环。该环很可能是在渐近的巨大分支相中喷出的气体,随后它被中心恒星的辐射光解离。 H I辐射的径向速度传播范围约为50 km s-1。 H I的质量为〜0.07 M 4,是分子氢质量的约3倍,与离子化氢的质量相当。
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