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Serpens and Supernova remnant

Shortcuts: Differences, Similarities, Jaccard Similarity Coefficient, References.

Difference between Serpens and Supernova remnant

Serpens vs. Supernova remnant

Serpens ("the Serpent", Greek Ὄφις) is a constellation of the northern hemisphere. A supernova remnant (SNR) is the structure resulting from the explosion of a star in a supernova.

Similarities between Serpens and Supernova remnant

Serpens and Supernova remnant have 11 things in common (in Unionpedia): Hydrogen, Neutron star, Oxygen, Planetary nebula, Pulsar, Pulsar wind nebula, SN 1987A, Supernova, Synchrotron radiation, White dwarf, X-ray.

Hydrogen

Hydrogen is a chemical element with symbol H and atomic number 1.

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Neutron star

A neutron star is the collapsed core of a large star which before collapse had a total of between 10 and 29 solar masses.

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Oxygen

Oxygen is a chemical element with symbol O and atomic number 8.

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Planetary nebula

A planetary nebula, abbreviated as PN or plural PNe, is a type of emission nebula consisting of an expanding, glowing shell of ionized gas ejected from red giant stars late in their lives.

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Pulsar

A pulsar (from pulse and -ar as in quasar) is a highly magnetized rotating neutron star or white dwarf that emits a beam of electromagnetic radiation.

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Pulsar wind nebula

A pulsar wind nebula (PWN, plural PWNe), sometimes called a plerion (derived from the Greek "πλήρης", pleres, meaning "full"), is a type of nebula found inside the shells of supernova remnants (SNRe) that is powered by pulsar winds generated by its central pulsar.

Pulsar wind nebula and Serpens · Pulsar wind nebula and Supernova remnant · See more »

SN 1987A

SN 1987A was a peculiar type II supernova in the Large Magellanic Cloud, a dwarf galaxy satellite of the Milky Way.

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Supernova

A supernova (plural: supernovae or supernovas, abbreviations: SN and SNe) is a transient astronomical event that occurs during the last stellar evolutionary stages of a star's life, either a massive star or a white dwarf, whose destruction is marked by one final, titanic explosion.

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Synchrotron radiation

Synchrotron radiation (also known as magnetobremsstrahlung radiation) is the electromagnetic radiation emitted when charged particles are accelerated radially, i.e., when they are subject to an acceleration perpendicular to their velocity.

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White dwarf

A white dwarf, also called a degenerate dwarf, is a stellar core remnant composed mostly of electron-degenerate matter.

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X-ray

X-rays make up X-radiation, a form of electromagnetic radiation.

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The list above answers the following questions

Serpens and Supernova remnant Comparison

Serpens has 228 relations, while Supernova remnant has 43. As they have in common 11, the Jaccard index is 4.06% = 11 / (228 + 43).

References

This article shows the relationship between Serpens and Supernova remnant. To access each article from which the information was extracted, please visit:

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