Data collected by the Arecibo Radio Telescope before it collapsed late last year will help astronomers better understand how our local neighbourhood of galaxies formed.
Arecibo was the world’s largest single-dish radio telescope until it was surpassed in 2016 by China’s Five-hundred-meter Aperture Spherical Telescope (FAST). At the end of 2020, Arecibo’s 900-ton receiver platform suddenly and spectacularly fell onto the dish below, destroying the telescope.
A team of astronomers from the University of Western Australia and the International Centre for Radio Astronomy Research (ICRAR) in Perth have used Arecibo’s observations of nearby galaxies to test the ‘Fall relation’.
First presented by S. Michael Fall in 1983, the Fall relation suggests the mass of stars belonging to a galaxy and its rotation directly correlate to each other and dictate how a galaxy will grow and evolve.
Funded by the Australian Research Council and published in the journal Monthly Notices of the Royal Astronomical Society (MNRAS), the new study tests this relationship using data collected from 564 galaxies of varying shapes and ages, making it the largest representative sample of its kind.
Lead author and PhD candidate Jennifer Hardwick said the study would help researchers better understand how a wide range of galaxies evolved and formed, including our galaxy, the Milky Way.
“Although the Fall relation was first suggested almost 40 years ago, previous research to refine its properties had small samples and was limited in the types of galaxies used,” Hardwick said.
“This work challenges astronomers’ current understanding of how galaxies change over their lifetime and provides a constraint for future researchers to develop these theories further.”
Prior research into this relationship has been restricted by the type and number of known galaxies with resolved accurate data, which researchers use to measure galaxy rotation through the Doppler effect.
The study shows that the relationship between the mass of stars and a galaxy’s rotation is not what we first thought, with different galaxy types displaying a different relationship between the two properties.
“Because galaxies evolve over billions of years, we have to work with snapshots of their evolution— taken from different stages of their life—and try to piece together their journey.”
This process has left astronomers with lots of unanswered questions about a galaxy’s lifecycle.
“By developing a better understanding of galaxies properties now, we can incorporate these into our simulations to work backwards,” she said.
Associate Professor Luca Cortese, Ms Hardwick’s supervisor and co-author, said the study shows the importance of revisiting research as our technology advances.
“This creates a cycle of technological development, resulting in new discoveries which push for further advances,” he said. “However, before getting to the new discoveries, it is critical to revisit previous knowledge to make sure that our foundations are correct.
“Since the dawn of extragalactic astronomy, it was clear that angular momentum is a key property for understanding how galaxies form and evolve. However, due to the difficulty of measuring angular momentum, direct observational constraints to our theory have been lacking.
“This work provides an important reference for future studies, offering one of the best measurements of the connection between angular momentum and other galaxy properties in the local Universe.”
The research also reinforces the importance of the Arecibo Radio Telescope to astronomy over the past 58 years, even after its forced retirement in 2020.
“Despite the fact that the Arecibo Radio Telescope suddenly collapsed last year, observations of atomic hydrogen content in galaxies carried out with this facility still provide the deepest census of gas content in galaxies,” Associate Professor Cortese said.
“We will have to wait for the second half of this decade before these kinds of observations are superseded by data obtained with the precursors of the Square Kilometre Array, such as Australia’s SKA Pathfinder Telescope (ASKAP), South Africa’s Karoo Array Telescope (MeerKAT) and China’s Five-hundred-meter Aperture Spherical radio Telescope (FAST).”
‘xGASS: Characterising the slope and scatter of the stellar mass – angular momentum relation for nearby galaxies’, published in Monthly Notices of the Royal Astronomical Society on December 1st, 2021.
The International Centre for Radio Astronomy Research (ICRAR) is a joint venture between Curtin University and The University of Western Australia with support and funding from the State Government of Western Australia.
The Galaxy Evolution Explorer (GALEX) was an orbiting ultraviolet space telescope that was launched on 28 April 2003 and operated until early 2012 (decommissioned in June 2013).
The Arecibo Telescope was a 305-metre spherical reflector radio telescope built into a natural sinkhole at the Arecibo Observatory located in Puerto Rico. Completed in 1963, it was the world’s largest single-aperture telescope until it was surpassed in 2016 by the Five-hundred-meter Aperture Spherical Telescope (FAST) in Guizhou, China. At the end of 2020, after years of maintenance issues, Arecibo’s 900-ton receiver platform fell onto the reflector dish below, destroying the telescope.
The extended GALEX Arecibo SDSS Survey (xGASS)
The extended GALEX Arecibo SDSS Survey (xGASS) measured the neutral hydrogen content of a sample of ~1200 galaxies using the Arecibo radio telescope. Targets were selected from the Sloan Digital Sky Survey (SDSS) spectroscopic and Galaxy Evolution Explorer (GALEX) imaging surveys, which provided uniform measurements of their stellar and star formation properties. xGASS includes the deepest observations of atomic hydrogen in galaxies in the local Universe available to date.
Jennifer Hardwick (ICRAR / University of Western Australia)
Ph: +61 407 046 764 E: Jennifer.Hardwick@icrar.org
A/Prof. Luca Cortese (ICRAR / University of Western Australia)
Ph: +61 8 6488 3663 E: Luca.Cortese@icrar.org
Pete Wheeler (Media Contact, ICRAR)
Ph: +61 0423 982 018 E: Pete.Wheeler@icrar.org