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.
Hydrogen and Serpens · Hydrogen and Supernova remnant ·
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.
Neutron star and Serpens · Neutron star and Supernova remnant ·
Oxygen
Oxygen is a chemical element with symbol O and atomic number 8.
Oxygen and Serpens · Oxygen and Supernova remnant ·
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.
Planetary nebula and Serpens · Planetary nebula and Supernova remnant ·
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.
Pulsar and Serpens · Pulsar and Supernova remnant ·
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 ·
SN 1987A
SN 1987A was a peculiar type II supernova in the Large Magellanic Cloud, a dwarf galaxy satellite of the Milky Way.
SN 1987A and Serpens · SN 1987A and Supernova remnant ·
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.
Serpens and Supernova · Supernova and Supernova remnant ·
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.
Serpens and Synchrotron radiation · Supernova remnant and Synchrotron radiation ·
White dwarf
A white dwarf, also called a degenerate dwarf, is a stellar core remnant composed mostly of electron-degenerate matter.
Serpens and White dwarf · Supernova remnant and White dwarf ·
X-ray
X-rays make up X-radiation, a form of electromagnetic radiation.
The list above answers the following questions
- What Serpens and Supernova remnant have in common
- What are the similarities between Serpens and Supernova remnant
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
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