Why massive galaxies don't dance in crowds

Why massive galaxies don’t dance in crowds
Galaxy cluster Abell 2744, imaged with the Hubble Space Telescope. The cluster lies in the constellation of Sculptor and contains several hundred galaxies. Credit: NASA, ESA, and R. Dupke (Eureka Scientific, Inc.), et al.

Scientists have discovered why heavyweight galaxies living in a dense crowd of galaxies tend to spin more slowly than their lighter neighbours.

"Contrary to earlier thinking, the spin rate of the galaxy is determined by its mass, rather than how crowded its neighbourhood is," says study first author Associate Professor Sarah Brough of UNSW Sydney and the ARC Centre of Excellence for All-sky Astrophysics, CAASTRO.

The finding, based on a detailed study of more than 300 , is published in the Astrophysical Journal.

To measure how fast their galaxies rotated, the researchers used an instrument called the Sydney-AAO Multi-object Integral field spectrograph (SAMI) on the 4-metre Anglo-Australian Telescope in eastern Australia.

SAMI 'dissects' galaxies, obtaining optical spectra from 61 points across the face of each galaxy, 13 galaxies at a time.

"We want to know which factors really drive how galaxies evolve," says team member Dr Matt Owers of the Australian Astronomical Observatory and Macquarie University. "In this case, we've sorted out nature versus nurture."

The new finding runs counter to previous studies, made with smaller samples of galaxies, which concluded that a galaxy's spin rate is determined by the other galaxies in its neighbourhood.

Associate Professor Brough says this earlier conclusion was spurious. "Once you take into account the strong association with mass, there's no link between a galaxy's spin rate and its environment," she says.

Credit: University of New South Wales

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More information: Sarah Brough et al. The SAMI Galaxy Survey: Mass as the Driver of the Kinematic Morphology–Density Relation in Clusters, The Astrophysical Journal (2017). DOI: 10.3847/1538-4357/aa7a11
Journal information: Astrophysical Journal

Citation: Why massive galaxies don't dance in crowds (2017, August 10) retrieved 18 August 2019 from https://phys.org/news/2017-08-massive-galaxies-dont-crowds.html
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Aug 11, 2017
I think the most important phrase in the whole story is the words: "Contrary to earlier thinking"

That is the most important type of observation scientists can make as it overturns false data and false thinking which permeates and pervades our scientific data and discourse.

Aug 11, 2017
That is the most important type of observation scientists can make as it overturns false data and false thinking which permeates and pervades our scientific data and discourse
sigh
1- all science is on the frontiers of knowledge (important to remember)

2- colourful adjectives are not representative of all science, only reporting (and not always accurate)

3- you have absolutely no evidence that science, it's data or discourse, is permeated with false data or false thinking
this is important to note because it is demonstrative of your lack of science literacy on many levels: just because a point changes a hypothesis or adjusts data to make something more accurate doesn't mean it falsifies previous points or data

example: GR/SR
it also was "Contrary to earlier thinking", however we still use Newtonian physics


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