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HST Imaging of Proto-Planetary and Very Young Planetary Nebulae Towards a New Understanding of Their Formation

机译：原行星和非常年轻行星状星云的HsT成像对其形成的新认识

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Sahai, R.;
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年度 2000
页码 1-15
总页数 15
原文格式 PDF
正文语种 eng
中图分类工业技术;
关键词
IMAGING TECHNIQUES; LOSSES; NEBULAE; PLANETARY NEBULAE; STELLAR EVOLUTION; Mass-Loss Late Stellar Evolution Protoplanetary Nebulae Planetary Nebulae;

机译：成像技术;损失;星云; pLaNETaRY NEBULaE; sTELLaR EVOLUTION;质量损失晚恒星演化原行星云星云行星状星云;

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专利

1. H2 Imaging of Three Proto-Planetary and Young Planetary Nebulae* [J] . Kevin Volk1, Bruce J. Hrivnak2, Sun Kwok3 The Astrophysical journal . 2008,第2期

机译：三个原始行星和年轻行星状星云的H2成像*
2. SHAPING PROTO-PLANETARY AND YOUNG PLANETARY NEBULAE WITH COLLIMATED FAST WINDS [J] . CHIN-FEI LEE, RAGHVENDRA SAHAI The Astrophysical journal . 2003,第1aaParta1期

机译：用集合的快速风塑造原行星和幼行星星云
3. SHAPING PROTO-PLANETARY AND YOUNG PLANETARY NEBULAE WITH COLLIMATED FAST WINDS [J] . CHIN-FEI LEE, RAGHVENDRA SAHAI The Astrophysical journal . 2003,第1aPta1期

机译：用集合的快速风塑造原行星和年轻的行星状星云
4. Very Young Proto-Planetary Nebulae: An Optical Imaging and Spectroscopic Survey [C] . Sahai R., Sanchez Contreras C. Meeting on Asymmetrical planetary nebulae . 2004

机译：非常年轻的ProDo-Planetary星云：光学成像和光谱调查
5. Hubble space telescope observations of proto-planetary nebulae. [D] . Su, Kate Yu Ling. 2000

机译：哈勃太空望远镜对原行星云的观测。
6. Nebular and auroral emission lines of Cl iii in the optical spectra of planetary nebulae [O] . Francis P. Keenan, Lawrence H. Aller, Catherine A. Ramsbottom, 2000

机译：Cl iii的神经和极光发射线行星状星云的光谱
7. HST/NICMOS Imaging Polarimetry of Proto-Planetary Nebulae II: Macro-morphology of the Dust Shell Structure via Polarized Light [O] . Ueta, Toshiya, Murakawa, Koji, Meixner, Margaret 2007

机译：原行星星云II的HsT / NICmOs成像偏振测量：通过偏振光对尘壳结构的宏观形态
8. Bipolar Bubbles, Jets and Rings in Very Low Excitation Planetary Nebulae - First Results for an HST/WFPC2 Imaging Survey [R] . Sahai, R., Trauger, J. 1997

机译：极低激发行星状星云中的双极气泡，喷流和环 - HsT / WFpC2成像调查的第一个结果

HST Imaging of Proto-Planetary and Very Young Planetary Nebulae Towards a New Understanding of Their Formation

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