Objects with variable star designations

variable star in the constellation Auriga

variable star in the constellation Monoceros

nova in the constellation Centaurus

star

star in the constellation Cassiopeia

star in the constellation Cygnus

star in the constellation Boötes

star in the constellation Andromeda

star in the constellation Canis Major

star

star in the constellation Boötes

star in the constellation Aquila

star in the constellation Pictor

OGLE-TR-122 is a binary stellar system containing one of the smallest main-sequence stars whose radius has been measured. It was discovered when the Optical Gravitational Lensing Experiment (OGLE) survey observed the smaller star eclipsing the larger primary. The orbital period is approximately 7.3 days. The system's primary is thought to resemble the Sun. ==OGLE-TR-122B== thumb|left|Brightness dip and velocity variations of OGLE-TR-122 The smaller star, OGLE-TR-122B, is estimated to have a radius around 0.12 solar radii, or around 20% larger than Jupiter's, and a mass of around 0.1 solar mas

pulsating variable star in the constellation Scutum

binary star in the constellation Camelopardalis

variable star in the constellation Lepus

star in the constellation Orion

variable star in the constellation Cetus

variable star in the constellation Sagitta

star in the constellation Andromeda

star

star

star

star in the constellation Aquila

star in the constellation Canes Venatici

variable star in the constellation Aries

binary star in the constellation Auriga

variable star in the constellation Auriga

OGLE-TR-113 is a dim, distant magnitude 16 binary star in the star fields of the constellation Carina. Because of its distance of about 1,930 light years, and location in a crowded field it was not notable in any way. Its apparent brightness changes when one of its planets transits, so the star has been given the variable star designation V752 Carinae. Spectral type of the star is type K dwarf star, slightly cooler and less luminous than the Sun.

binary star in the constellation Corvus

recurrent nova

star in the constellation Pisces

star in the constellation Auriga

variable star in the constellation Orion

star in the constellation Vulpecula

Rotating variable star in the constellation Carina

star in the constellation Leo Minor

star in the constellation Cassiopeia

variable star in the constellation Vulpecula

star in the constellation Canes Venatici

binary star system in the constellation Perseus

star in the constellation Boötes

variable star in the constellation Aquila

star in the constellation Hercules

star in the constellation Ursa Major

star in the constellation Aquila

WASP-3 is a triple star system located about away from the Sun in the constellation Lyra. The system has an apparent magnitude of 10. The brightest and most massive star of this system is WASP-3A, an F-type main sequence star which has one known transiting hot Jupiter exoplanet, WASP-3b. Since the planet transits the star, the star is classified as a planetary transit variable and has received the variable star designation V838 Lyrae.

star in the constellation Aquarius

star in the constellation Serpens

star in the constellation Cetus

star in the constellation Pyxis

star in the constellation Gemini

star in the constellation Sagitta

star

variable star in the constellation Horologium

Star in the constellation Cygnus

star in the constellation Aries

variable star in the constellation Carina

star in the constellation Cygnus