英语词汇“nebular”的意思、用法、释义、翻译、读音、例句、短语、词组-英语词典

是什么意思

adj.

星云的；

英英释义

nebular[ 'nebjul? ]

adj.
- of or relating to or resembling a nebula
  "the nebular hypothesis of the origin of the solar system"
  同义词：nebulous
- resembling a cloud
  同义词：cloudlike

学习怎么用

双语例句

用作形容词(adj.)

The remnant nebular gas pervades the interplanetary space.
星云的残余气体充斥星际空间。

权威例句

X-ray nebular models
Nebular emission from star-forming galaxies
Infrared Observations of Nebular Emission Lines from Galaxies at z 3
Optical Spectroscopy and Nebular Oxygen Abundances of the Spitzer/SINGS Galaxies
On Measuring Nebular Chemical Abundances in Distant Galaxies Using Global Emission-Line Spectra
The Evolution of Viscous Discs and the Origin of the Nebular Variables
Electron temperature variations and the measurement of nebular abundances
Mineralogical and chemical modification of components in CV3 chondrites: Nebular or asteroidal processing?
The WC10 central stars CPD - 56° 8032 and He 2-113 – II. Model analysis and comparison with nebular properties
The Composition Gradient in M101 Revisited. II. Electron Temperatures and Implications for the Nebular Abundance Scale

单词	nebular
释义	nebular 听听怎么读英 ['nebj?l?] 美 ['nebj?l?] 是什么意思 adj. 星云的；英英释义 nebular[ 'nebjul? ] adj. of or relating to or resembling a nebula "the nebular hypothesis of the origin of the solar system" 同义词：nebulous resembling a cloud 同义词：cloudlike 学习怎么用双语例句用作形容词(adj.) The remnant nebular gas pervades the interplanetary space. 星云的残余气体充斥星际空间。权威例句 X-ray nebular models Nebular emission from star-forming galaxies Infrared Observations of Nebular Emission Lines from Galaxies at z 3 Optical Spectroscopy and Nebular Oxygen Abundances of the Spitzer/SINGS Galaxies On Measuring Nebular Chemical Abundances in Distant Galaxies Using Global Emission-Line Spectra The Evolution of Viscous Discs and the Origin of the Nebular Variables Electron temperature variations and the measurement of nebular abundances Mineralogical and chemical modification of components in CV3 chondrites: Nebular or asteroidal processing? The WC10 central stars CPD - 56° 8032 and He 2-113 – II. Model analysis and comparison with nebular properties The Composition Gradient in M101 Revisited. II. Electron Temperatures and Implications for the Nebular Abundance Scale
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