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Ten billion years of brightest cluster galaxy alignments
Tekijät: West MJ, De Propris R, Bremer MN, Phillipps S
Kustantaja: NATURE PUBLISHING GROUP
Julkaisuvuosi: 2017
Journal: Nature Astronomy
Tietokannassa oleva lehden nimi: NATURE ASTRONOMY
Lehden akronyymi: NAT ASTRON
Artikkelin numero: ARTN 0157
Vuosikerta: 1
Numero: 7
Sivujen määrä: 4
ISSN: 2397-3366
DOI: https://doi.org/10.1038/s41550-017-0157
Tiivistelmä
A galaxy's orientation is one of its most basic observable properties. Astronomers once assumed that galaxies are randomly oriented in space; however, it is now clear that some have preferred orientations with respect to their surroundings. Chief among these are giant elliptical galaxies found in the centres of rich galaxy clusters. Numerous studies have shown that the major axes of these galaxies often share the same orientation as the surrounding matter distribution on larger scales(1-6). Using Hubble Space Telescope observations of 65 distant galaxy clusters, we show that similar alignments are seen at earlier epochs when the Universe was only one-third of its current age. These results suggest that the brightest galaxies in clusters are the product of a special formation history, one influenced by development of the cosmic web over billions of years.
A galaxy's orientation is one of its most basic observable properties. Astronomers once assumed that galaxies are randomly oriented in space; however, it is now clear that some have preferred orientations with respect to their surroundings. Chief among these are giant elliptical galaxies found in the centres of rich galaxy clusters. Numerous studies have shown that the major axes of these galaxies often share the same orientation as the surrounding matter distribution on larger scales(1-6). Using Hubble Space Telescope observations of 65 distant galaxy clusters, we show that similar alignments are seen at earlier epochs when the Universe was only one-third of its current age. These results suggest that the brightest galaxies in clusters are the product of a special formation history, one influenced by development of the cosmic web over billions of years.
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