G 185-32

G 185-32, also known by the variable star designation PY Vulpeculae, is a white dwarf in the constellation Vulpecula. ^[1]

17 relations: Ambri Airport, American Association of Variable Star Observers, Apparent magnitude, California Institute of Technology, Constellation, Gliese Catalogue of Nearby Stars, Henry L. Giclas, Jesse L. Greenstein, Light curve, Lowell Observatory, Proper motion, Pulsating white dwarf, Star catalogue, United States Naval Observatory, Variable-star designation, Vulpecula, White dwarf.
Pulsating white dwarfs
White dwarf star stubs

Ambri Airport

Ambri Airport (ICAO: LSPM) is a Swiss general aviation airport.

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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.

See G 185-32 and Apparent magnitude

California Institute of Technology

The California Institute of Technology (branded as Caltech) is a private research university in Pasadena, California.

See G 185-32 and California Institute of Technology

Constellation

A constellation is an area on the celestial sphere in which a group of visible stars forms a perceived pattern or outline, typically representing an animal, mythological subject, or inanimate object.

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Gliese Catalogue of Nearby Stars

The Gliese Catalogue of Nearby Stars (English) is a star catalogue listing stars located within 25 parsecs (82 ly) of the Sun.

See G 185-32 and Gliese Catalogue of Nearby Stars

Henry L. Giclas

Henry Lee Giclas (December 9, 1910 – April 2, 2007) was an American astronomer and a discoverer of minor planets and comets.

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Jesse L. Greenstein

Jesse Leonard Greenstein (October 15, 1909 – October 21, 2002) was an American astronomer.

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In astronomy, a light curve is a graph of the light intensity of a celestial object or region as a function of time, typically with the magnitude of light received on the y-axis and with time on the x-axis.

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Lowell Observatory

Lowell Observatory is an astronomical observatory in Flagstaff, Arizona, United States.

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Proper motion

Proper motion is the astrometric measure of the observed changes in the apparent places of stars or other celestial objects in the sky, as seen from the center of mass of the Solar System, compared to the abstract background of the more distant stars.

See G 185-32 and Proper motion

Pulsating white dwarf

A pulsating white dwarf is a white dwarf star whose luminosity varies due to non-radial gravity wave pulsations within itself. G 185-32 and pulsating white dwarf are pulsating white dwarfs.

See G 185-32 and Pulsating white dwarf

Star catalogue

A star catalogue is an astronomical catalogue that lists stars.

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United States Naval Observatory

The United States Naval Observatory (USNO) is a scientific and military facility that produces geopositioning, navigation and timekeeping data for the United States Navy and the United States Department of Defense.

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Variable-star designation

In astronomy, a variable-star designation is a unique identifier given to variable stars. G 185-32 and variable-star designation are objects with variable star designations.

See G 185-32 and Variable-star designation

Vulpecula

Vulpecula is a faint constellation in the northern sky.

See G 185-32 and Vulpecula

White dwarf

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

See G 185-32 and White dwarf

References

[1] https://en.wikipedia.org/wiki/G_185-32

Also known as PY Vulpeculae.

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