We present high-resolution, spatially resolved spectra of the nebula surrounding Sakurai's object. We find the expansion velocity of the nebula to be 30.9 ± 0.7 km s-1, and the nebula extent to be 44'' in diameter. We discuss the wide range of reported distances to Sakurai's object and the dilemma that these present, since some evidence strongly favors a short distance (1.1 kpc) while other data strongly favor a longer distance (5–8 kpc). We also present spectra of Sakurai's star centered near the λ4216 CN band that suggests the star had cooled significantly between 1996 October and 1997 May, but had not cooled further by 1997 July.
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机译:我们提出了樱井天体周围星云的高分辨率,空间分辨光谱。我们发现星云的膨胀速度为30.9±0.7 km s-1,星云的直径为44英寸。我们讨论了所报告的到樱井目标的距离的广泛范围以及这些距离所带来的困境,因为一些证据强烈赞成短距离(1.1 kpc),而其他数据强烈赞成更长的距离(5-8 kpc)。我们还给出了樱井星的光谱,其中心位于λ4216CN波段附近,这表明该恒星在1996年10月至1997年5月之间已显着冷却,但在1997年7月之前并未进一步冷却。
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