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1.From AGB Star to Planetary Nebula
从AGB星到行星状星云收藏指正
2.The Drastic Disappearance of Eclipses in the Central Star of the Planetary Nebula NGC 2345
行星状星云NGC2346核星的食光变现象的消失收藏指正
3.[Left] — A towering "mountain" of cold hydrogen gas laced with dust is the site of new star formation in the Carina Nebula.
左图——一个饰有尘埃花边高耸的冷氢气“山脉”正是船底座星云中新恒星诞生地。收藏指正
4.This Hubble Space Telescope view of the central region of the Carina Nebula reveals a violent maelstrom of star birth.
此次“哈勃”空间望远镜对船底座星云中心区域的观察展现了一场狂暴的恒星诞生风潮。收藏指正
5.a nebula that was once thought to be a star with its planets but is now thought to be a very hot star surrounded by an expanding envelope of ionized gases that emit a fluorescent glow because of intense radiation from the star.
一个原本被认为是带行星的恒星的星云，现在被认为是非常热的恒星，由扩大的离子态气体包层包围，由于恒星的剧烈辐射放射出光和热。收藏指正
6.In looking at the Carina Nebula we are seeing the genesis of star making as it commonly occurs along the dense spiral arms of a galaxy.
通过对船底座星云的观察，我们看到了通常沿银河密集的旋臂所诞生恒星的起源。收藏指正
7.We present H and K s polarimetric images in a ～5′ field of star forming region NGC7538. The polarimetric images reveal the complex structure of infrared nebulosities and clusters of young stars, associated with the bright infrared sources IRS 1 11. The polarization pattern in the IRS 1 3 nebula shows a dominant illumination from deeply embedded source IRS 1. The morphology of the nebula can be modeled by a low extincted bubble enclosed by redder and highly polarized shell.
介绍恒星形成区NGC7538的H和Ks波段偏振成像的观测结果．近5′视场的偏振图像揭示了与亮红外源IRS1?11成协的年轻星团和红外星云的复杂结构．IRS1?3星云的偏振图像表明星云的近红外辐射主要来自对深埋红外源IRS1的反射；收藏指正
8.Unlike the rapidly rotating neutron stars in the Crab Nebula and Vela supernova remnants that are surrounded by dynamic magnetized clouds of electrons called pulsar wind nebulas, this neutron star is quiet, faint, and so far shows no evidence for pulsed radiation.
与蟹状星云和船帆座超新星遗迹中被磁化电子云（脉冲星风星云）环绕的高速自转中子星不同，这颗中子星安静而虚弱，目前为止，没有显示脉冲辐射的迹象。收藏指正
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