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Publication

The GOGREEN Survey: A deep stellar mass function of cluster galaxies at 1.0 < z < 1.4 and the complex nature of satellite quenching

Pascale Jablonka, Hung-Hsu Chan
2020
Journal Articles

Abstract

We study the stellar mass functions (SMFs) of star-forming and quiescent galaxies in 11 galaxy clusters at 1.0

Official source

https://infoscience.epfl.ch/entities/publication/330a7077-0678-4c02-899d-c4e368665d64

About this result

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Pascale Jablonka, Hung-Hsu Chan
2020
Journal Articles

Abstract

We study the stellar mass functions (SMFs) of star-forming and quiescent galaxies in 11 galaxy clusters at 1.0

Official source

https://infoscience.epfl.ch/entities/publication/330a7077-0678-4c02-899d-c4e368665d64

About this result

Ontological neighbourhood

Astronomy

Astrophysics: Stellar astronomy

Related concepts (31)

Star cluster

Star clusters are large groups of stars held together by self-gravitation. Two main types of star clusters can be distinguished: globular clusters are tight groups of ten thousand to millions of old stars which are gravitationally bound, while open clusters are more loosely clustered groups of stars, generally containing fewer than a few hundred members, and are often very young.

Star formation

Star formation is the process by which dense regions within molecular clouds in interstellar space, sometimes referred to as "stellar nurseries" or "star-forming regions", collapse and form stars. As a branch of astronomy, star formation includes the study of the interstellar medium (ISM) and giant molecular clouds (GMC) as precursors to the star formation process, and the study of protostars and young stellar objects as its immediate products. It is closely related to planet formation, another branch of astronomy.

Star

A star is an astronomical object comprising a luminous spheroid of plasma held together by self-gravity. The nearest star to Earth is the Sun. Many other stars are visible to the naked eye at night; their immense distances from Earth make them appear as fixed points of light. The most prominent stars have been categorised into constellations and asterisms, and many of the brightest stars have proper names. Astronomers have assembled star catalogues that identify the known stars and provide standardized stellar designations.

Related publications (47)

The GOGREEN Survey: A deep stellar mass function of cluster galaxies at 1.0 < z < 1.4 and the complex nature of satellite quenching

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Distinct origins of environmentally quenched galaxies in the core and outer virialised regions of massive clusters at 0.8 &lt; z &lt; 1.5

Evolution of the UV slope of galaxies at cosmic morning (z > 4): The properties of extremely blue galaxies

BEACON: JWST NIRCam Pure-parallel Imaging Survey. I. Survey Design and Initial Results

The GOGREEN Survey: A deep stellar mass function of cluster galaxies at 1.0 < z < 1.4 and the complex nature of satellite quenching

Distinct origins of environmentally quenched galaxies in the core and outer virialised regions of massive clusters at 0.8 &amp;lt; z &amp;lt; 1.5

Evolution of the UV slope of galaxies at cosmic morning (z > 4): The properties of extremely blue galaxies

BEACON: JWST NIRCam Pure-parallel Imaging Survey. I. Survey Design and Initial Results

Distinct origins of environmentally quenched galaxies in the core and outer virialised regions of massive clusters at 0.8 < z < 1.5