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emission nebula


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'emission nebula' can also refer to...

emission nebula

Molecular hydrogen line emission from the reflection nebula Parsamyan 18

On the magnetohydrodynamic modelling of the Crab nebula radio emission

Predicted radio-continuum emission from the little Homunculus of the η Carinae nebula

Modelling the warm H2 infrared emission of the Helix nebula cometary knots

What produces the diffuse X-ray emission from the Orion nebula? I. Simple spherical models

The emission and kinematic structures of the bipolar planetary nebula M 1-8

Suzaku Observation of Diffuse X-Ray Emission from the Carina Nebula

H2O maser emission associated with the planetary nebula IRAS 16333−4807

Unlocking the Keyhole: H2 and PAH emission from molecular clumps in the Keyhole Nebula

The nature and structure of the emission line nebula K 3-35: a very young planetary nebula with precessing bipolar jet-like outflows?

H110α recombination-line emission and 4.8-GHz continuum emission in the Carina nebula

Three-dimensional numerical model of the Omega Nebula (M17): simulated thermal X-ray emission

The impact of the nitrogen-to-oxygen ratio on ionized nebula diagnostics based on [N ii] emission lines

Suzaku and XMM-Newton Observations of Diffuse X-Ray Emission from the Eastern Tip Region of the Carina Nebula

Spectral Variation of Hard X-Ray Emission from the Crab Nebula with the Suzaku Hard X-Ray Detector

Imaging study of NGC 3372, the Carina nebula – III. The properties of G287.47−0.54 (Tr 14-N4), an embedded young cluster and its associated H2 emission*

 

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A luminous cloud of gas and dust in space which shines with its own light. The light can be generated in several ways. Usually the gas glows because it is exposed to a source of ultraviolet radiation; examples are H II regions and planetary nebulae, which are ionized by central stars. Gas may also glow because it has become ionized in a violent collision with another gas cloud, as in Herbig–Haro objects. Finally, some of the light from supernova remnants such as the Crab Nebula is produced by the process of synchrotron radiation, in which charged particles spiral around the interstellar magnetic field.

Subjects: Astronomy and Astrophysics.


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