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Symbiotic nova

Index Symbiotic nova

Symbiotic novae are slow irregular eruptive variable stars with very slow nova-like outbursts with an amplitude of between 9 and 11 magnitudes. [1]

10 relations: AG Pegasi, List of stars in Telescopium, Musca, Nova, RR Telescopii, Serpens, Southern Crab Nebula, SY Muscae, Symbiotic binary, Telescopium.

AG Pegasi

AG Pegasi is a symbiotic binary star in the constellation Pegasus.

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List of stars in Telescopium

This is the list of notable stars in the constellation Telescopium, sorted by decreasing brightness.

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Musca

Musca is a small constellation in the deep southern sky.

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Nova

A nova (plural novae or novas) or classical nova (CN, plural CNe) is a transient astronomical event that causes the sudden appearance of a bright, apparently "new" star, that slowly fades over several weeks or many months.

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RR Telescopii

RR Telescopii is a symbiotic nova in the southern constellation Telescopium.

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Serpens

Serpens ("the Serpent", Greek Ὄφις) is a constellation of the northern hemisphere.

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Southern Crab Nebula

The Southern Crab Nebula or Hen 2-104 is a nebula in the constellation Centaurus.

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SY Muscae

SY Muscae is a binary star system in the constellation Musca composed of a red giant and a white dwarf.

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Symbiotic binary

A symbiotic binary is a type of binary star system, often simply called a symbiotic star.

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Telescopium

Telescopium is a minor constellation in the southern celestial hemisphere, one of twelve named in the 18th century by French astronomer Nicolas-Louis de Lacaille and one of several depicting scientific instruments.

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Redirects here:

Symbiotic novae star.

References

[1] https://en.wikipedia.org/wiki/Symbiotic_nova

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