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Q Cygni

Index Q Cygni

Q Cygni (Q Cyg), is a star located in the constellation Cygnus. [1]

Table of Contents

  1. 20 relations: Accretion disk, American Association of Variable Star Observers, Apparent magnitude, Bright Star Catalogue, Cataclysmic variable star, Cygnus (constellation), Durchmusterung, Johann Friedrich Julius Schmidt, Lacerta, Monthly Notices of the Royal Astronomical Society, Nebula, New General Catalogue, Nova, Orbit, Planetary nebula, Publications of the Astronomical Society of the Pacific, Star, The Astronomical Journal, White dwarf, 2MASS.

Accretion disk

An accretion disk is a structure (often a circumstellar disk) formed by diffuse material in orbital motion around a massive central body.

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American Association of Variable Star Observers

The American Association of Variable Star Observers (AAVSO) is an international nonprofit organization.

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Apparent magnitude

Apparent magnitude is a measure of the brightness of a star or other astronomical object.

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Bright Star Catalogue

The Bright Star Catalogue, also known as the Yale Catalogue of Bright Stars, Yale Bright Star Catalogue, or just YBS, is a star catalogue that lists all stars of stellar magnitude 6.5 or brighter, which is roughly every star visible to the naked eye from Earth. Q Cygni and bright Star Catalogue are bright Star Catalogue objects.

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Cataclysmic variable star

In astronomy, cataclysmic variable stars (CVs) are stars which irregularly increase in brightness by a large factor, then drop back down to a quiescent state.

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Cygnus (constellation)

Cygnus is a northern constellation on the plane of the Milky Way, deriving its name from the Latinized Greek word for swan.

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Durchmusterung

In astronomy, Durchmusterung or Bonner Durchmusterung (BD) is an astrometric star catalogue of the whole sky, published by the Bonn Observatory in Germany from 1859 to 1863, with an extension published in Bonn in 1886.

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Johann Friedrich Julius Schmidt

Johann Friedrich Julius Schmidt (25 October 1825 in Eutin, Germany – 7 February 1884 in Athens, Greece) was a German astronomer and geophysicist.

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Lacerta

Lacerta is one of the 88 modern constellations defined by the International Astronomical Union.

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Monthly Notices of the Royal Astronomical Society

Monthly Notices of the Royal Astronomical Society (MNRAS) is a peer-reviewed scientific journal in astronomy, astrophysics and related fields.

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Nebula

A nebula (cloud, fog;: nebulae, nebulæ, or nebulas) is a distinct luminescent part of interstellar medium, which can consist of ionized, neutral, or molecular hydrogen and also cosmic dust.

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New General Catalogue

The New General Catalogue of Nebulae and Clusters of Stars (abbreviated NGC) is an astronomical catalogue of deep-sky objects compiled by John Louis Emil Dreyer in 1888. Q Cygni and New General Catalogue are NGC objects.

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Nova

A nova (novae or novas) is a transient astronomical event that causes the sudden appearance of a bright, apparently "new" star (hence the name "nova", Latin for "new") that slowly fades over weeks or months. Q Cygni and nova are novae.

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Orbit

In celestial mechanics, an orbit (also known as orbital revolution) is the curved trajectory of an object such as the trajectory of a planet around a star, or of a natural satellite around a planet, or of an artificial satellite around an object or position in space such as a planet, moon, asteroid, or Lagrange point.

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Planetary nebula

A planetary nebula 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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Publications of the Astronomical Society of the Pacific

Publications of the Astronomical Society of the Pacific (often abbreviated as PASP in references and literature) is a monthly peer-reviewed scientific journal managed by the Astronomical Society of the Pacific.

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Star

A star is a luminous spheroid of plasma held together by self-gravity.

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The Astronomical Journal

The Astronomical Journal (often abbreviated AJ in scientific papers and references) is a peer-reviewed monthly scientific journal owned by the American Astronomical Society (AAS) and currently published by IOP Publishing.

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White dwarf

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

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2MASS

The Two Micron All-Sky Survey, or 2MASS, was an astronomical survey of the whole sky in infrared light. Q Cygni and 2MASS are 2MASS objects.

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References

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

Also known as HR 8296, NGC 7114, Nova Cygni 1876.