Publication

Gaia Data Release 2 Summary of the variability processing and analysis results

Stephan Morgenthaler, Lorenzo Diana, Mária Süveges
2018
Journal Articles

Abstract

Context. The Gaia Data Release 2 (DR2) contains more than half a million sources that are identified as variable stars.

Official source

https://infoscience.epfl.ch/entities/publication/dc402b79-0e4d-4571-a9ee-a4cc49f0707b

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Stephan Morgenthaler, Lorenzo Diana, Mária Süveges
2018
Journal Articles

Abstract

Context. The Gaia Data Release 2 (DR2) contains more than half a million sources that are identified as variable stars.

Official source

https://infoscience.epfl.ch/entities/publication/dc402b79-0e4d-4571-a9ee-a4cc49f0707b

About this result

Related concepts (31)

Variable star

A variable star is a star whose brightness as seen from Earth (its apparent magnitude) changes with time. This variation may be caused by a change in emitted light or by something partly blocking the light, so variable stars are classified as either: Intrinsic variables, whose luminosity actually changes; for example, because the star periodically swells and shrinks. Extrinsic variables, whose apparent changes in brightness are due to changes in the amount of their light that can reach Earth; for example, because the star has an orbiting companion that sometimes eclipses it.

Data

In common usage and statistics, data (USˈdætə; UKˈdeɪtə) is a collection of discrete or continuous values that convey information, describing the quantity, quality, fact, statistics, other basic units of meaning, or simply sequences of symbols that may be further interpreted formally. A datum is an individual value in a collection of data. Data is usually organized into structures such as tables that provide additional context and meaning, and which may themselves be used as data in larger structures.

Cepheid variable

A Cepheid variable (ˈsɛfi.ɪd,_ˈsiːfi-) is a type of variable star that pulsates radially, varying in both diameter and temperature. It changes in brightness, with a well-defined stable period and amplitude. Cepheids are important cosmic benchmarks for scaling galactic and extragalactic distances. A strong direct relationship exists between a Cepheid variable's luminosity and its pulsation period. This characteristic of classical Cepheids was discovered in 1908 by Henrietta Swan Leavitt after studying thousands of variable stars in the Magellanic Clouds.

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