Objects with variable star designations

star in the constellation Libra

binary star system in the constellation Ophiuchus

red dwarf star in the constellation Cancer

nearby flare star in constellation Aries

star in the constellation Centaurus

star in the constellation Sagitta

star in the constellation Hydra

star in the constellation Microscopium

variable star in the constellation Lepus

binary star

triple star system in the constellation Cetus

binary star in the constellation Cepheus

protoplanetary nebula in the constellation Puppis

star in the constellation Carina

star in the constellation Lacerta

triple star system in the constellation Cygnus

variable star in the constellation Orion

red supergiant

star in the constellation Perseus

star

binary star in the constellation Virgo

binary star in the constellation Ursa Major

Binary star system, first known microquasar

star in the constellation Crater

star in the constellation Piscis Austrinus

star in the constellation Aquila

star in the constellation Ophiuchus

binary system in the constellation Aquila

active galaxy, prototype of the BL Lacertae objects

nova in the constellation Sagittarius

OGLE-TR-56 is a dim, distant, magnitude 17 Sun-like star located approximately away in the constellation of Sagittarius. This star is listed as an eclipsing type variable star with the eclipse due to the passage of the planet as noted in the discovery papers. The eclipses were detected by the Optical Gravitational Lensing Experiment (OGLE) team analysing data collected in 2001.

bright nova occurring in 1975 in the constellation Cygnus

nova in the constellation Delphinus

A0620-00 (abbreviated from 1A 0620-00) is a binary star system in the constellation of Monoceros, with an apparent magnitude of 11.2.

variable star in the constellation Puppis

star in the constellation Taurus

star in the constellation Centaurus

variable star in the constellation Cepheus

variable star in the constellation Taurus

multiple star

star in the constellation Monoceros

variable star in the constellation Leo

star in the constellation Aries

star in the constellation Leo

binary star with an X-ray pulsar in the constellation Centaurus

T Tauri-type star

star in the constellation Pictor

variable star in the constellation Cygnus

wide binary system in the Lupus constellation

star in the constellation Aquila

variable star in the constellation Gemini

star in the constellation Leo

variable star in the constellation Aquarius

thumb|left|A light curve for OGLE-TR-10 showing the planet transit, adapted from Pont et al. (2007) OGLE-TR-10 is a distant G-type main sequence star located 4100 light years from Earth in the constellation of Sagittarius. It is located near the Galactic Center. This star is listed as an eclipsing type variable star with the eclipse due to the passage of the planet as noted in the discovery papers. The eclipses were detected by the Optical Gravitational Lensing Experiment (OGLE) team analysing data collected in 2001.

GSC 03549-02811 (sometimes referred to as Kepler-1, or either TrES-2A or TrES-2 parent star in reference to its exoplanet TrES-2b) is a binary star system containing a G-type main-sequence star similar to the Sun. This star is located approximately 704 light-years away in the constellation of Draco. The apparent magnitude of this star is 11.41, which means it is not visible to the naked eye but can be seen with a medium-sized amateur telescope on a clear dark night. The age of this star is about 5 billion years.

K-type bright giant star in the constellation of Carina

variable star in the constellation Orion

star in the constellation Hercules

star

variable star in the constellation Cassiopeia