In this way, all emission nebulae are wonderfully weird, as they reveal nature’s artistry across intangible tapestries. But some can be considered weird for other reasons, as we will explore in ...

K3-35 is an emission-line nebula that contains a bipolar precessing jet, which is the origin of strong emission from N +, emanating from a bright core 5,6.These structures are embedded in an ...

IN the course of a radio survey of bright emission nebulæ with the 1,500-ft. Sydney cross-aerial, some fourteen nebulæ were studied at a wave-length of 3.5 m. Six were probably observed in ...

Robert Williams, Edward B. Jenkins, Jack A. Baldwin, Brian Sharpee, Comparative Absorption and Emission Abundance Analyses of Nebulae: Ion Emission Densities for IC 418, Publications of the ...

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Emission nebulae, more specifically, are clouds of ionized gas. Mostly mostly comprised of hydrogen, these clouds also harbor noticeable quantities of helium, oxygen, and nitrogen (among others).

A bubbling region of stars both old and new lies some 160,000 light-years away in the constellation Dorado. This complex cluster of emission nebulae is known as N11, and was discovered by American ...

One of the largest emission nebulae in the far northern sky can be found in IC 1396, a bright glow in Cepheus that contains several complex objects. Among them are the red supergiant star Mu ...

Universe Today, "Nebulae: What Are They And Where Do They Come From?", accessed July 2022. The University of Utah, " Nebula ", accessed July 2022. Australia Telescope National Facility, " Star ...