Image Credit: NGC 4632, a potential polar ring galaxy showing a ring of gas oriented perpendicularly to the galaxy’s main spiral disk. Source: Jayanne English (University of Manitoba), Nathan Deg (Queen’s University) & WALLABY Survey, CSIRO / ASKAP, NAOJ / Subaru Telescope
A collaborative effort among international astronomers, which includes scientists from Queen’s University, has led to the identification of two candidate polar ring galaxies. The findings were published on September 13 in the scientific journal, Monthly Notices of the Royal Astronomical Society.
Nathan Deg and Kristine Spekkens, both affiliated with the Departments of Physics, Engineering Physics & Astronomy at Queen’s University, spearheaded the analysis. Data for the study were gathered using a telescope operated by CSIRO, Australia’s national science agency. The data consisted of hydrogen gas sky maps from over 600 galaxies and were part of CSIRO’s ASKAP radio telescope’s WALLABY survey. The researchers identified two galaxies that potentially possess a ring of stars and gas oriented perpendicularly to their main spiral disks.
Dr. Nathan Deg, the lead author of the study, stated, “These polar ring galaxies are visually striking celestial bodies. Our findings indicate that between one and three percent of nearby galaxies may possess such gaseous polar rings, a frequency much greater than what optical telescopes had suggested.”
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Historical Context and Ramifications
While polar ring galaxies have been observed in the past, these are the first such instances recorded using the ASKAP telescope situated at Inyarrimanha Ilgari Bundara, which is part of CSIRO’s Murchison radio astronomy observatory located in Wajarri Yamaji Country in Western Australia. These new observations, based solely on gas detections, imply that polar ring galaxies may be more prevalent than was previously assumed.
Dr. Kristine Spekkens, a professor with a cross-appointment from the Royal Military College, remarked, “The extensive and deep sky mapping conducted has serendipitously led us to discover features we did not anticipate, thus underscoring the tremendous value of this kind of exploration.”
Unveiling Galactic Evolution
Further study of these polar ring structures could provide valuable insights into the evolution of galaxies. A prevalent theory suggests that polar rings form when a larger galaxy absorbs a smaller one. If polar ring galaxies are indeed more common, this might indicate that such galactic mergers occur more frequently.
In addition, polar ring galaxies offer a new avenue for researching dark matter. They could potentially be used to investigate the shape and properties of the host galaxy’s dark matter.
Professor Lister Staveley-Smith, WALLABY Co-Principal Investigator and Interim Executive Director at ICRAR, noted, “The WALLABY survey is expected to be a significant resource for uncovering more such galaxies and complex systems in the future.”
Advanced Imaging Techniques
Jayanne English, a team member of the WALLABY research project and an expert in astronomical imaging at the University of Manitoba, crafted the first visuals of these gas-encompassed polar ring galaxies. She integrated optical and radio data from various telescopes, including the Subaru telescope in Hawaii for the spiral disk image and WALLABY data for the gaseous ring.
Dr. Bärbel Koribalski, Senior Principal Research Scientist at CSIRO, stated, “Our ASKAP radio telescope is generating an immense volume of data that will help in discovering numerous hydrogen-rich galaxies, including more peculiar structures like polar rings.”
Over two dozen collaborators from multiple countries participated in analyzing the data from WALLABY’s first public data release, culminating in the publication of the study. The team plans to corroborate these findings through additional observations, including usage of the MeerKAT radio telescope in South Africa.
Assistant Professor Barbara Catinella, WALLABY Co-Principal Investigator and co-author of the study, concluded, “One of the most exhilarating results from comprehensive surveys like WALLABY is stumbling upon the unexpected. These unusual galaxies with exquisite gaseous rings exemplify this phenomenon.”
Reference: “WALLABY pilot survey: The potential polar ring galaxies NGC 4632 and NGC 6156” by N Deg, R Palleske, K Spekkens, et al., published in Monthly Notices of the Royal Astronomical Society on 13 September 2023. DOI: 10.1093/mnras/stad2312
Frequently Asked Questions (FAQs) about polar ring galaxies
What is the main finding of the study led by researchers from Queen’s University?
The primary discovery is that polar ring galaxies, which feature a ring of stars and gas oriented perpendicularly to their main spiral disks, might be more prevalent than previously assumed. The researchers estimate that one to three percent of nearby galaxies may possess such gaseous polar rings.
Who were the main contributors to this research?
The research was a collaborative effort among international astronomers, but it was led by Nathan Deg and Kristine Spekkens, both of whom are affiliated with the Departments of Physics, Engineering Physics & Astronomy at Queen’s University. The team also included researchers from various countries and institutions.
What telescope and survey were primarily used for this research?
The study primarily used data obtained from CSIRO’s ASKAP radio telescope as part of the WALLABY survey. This telescope is located at Inyarrimanha Ilgari Bundara, part of CSIRO’s Murchison radio astronomy observatory in Western Australia.
Why are polar ring galaxies important for scientific research?
Polar ring galaxies can provide valuable insights into the evolution of galaxies. They can also offer new avenues for investigating the properties and distribution of dark matter in the host galaxies. Understanding these structures can have broader implications for the fields of astronomy and physics.
What are the future steps for this research?
The next step for the research team is to confirm their findings through additional observations, specifically by using different telescopes, including the MeerKAT radio telescope in South Africa.
What was the method used for visualizing these polar ring galaxies?
Jayanne English, an expert in astronomical imaging at the University of Manitoba, crafted the first visuals. She integrated optical and infrared data from the Subaru telescope in Hawaii for the spiral disk image and added the gaseous ring based on data from the WALLABY survey.
What is the significance of the WALLABY survey in this study?
The WALLABY survey is a project using CSIRO’s ASKAP radio telescope to detect atomic hydrogen emission from about half a million galaxies. The data from this survey contributed to the identification of the potential polar ring galaxies and will continue to be a valuable resource for future discoveries.
More about polar ring galaxies
- Monthly Notices of the Royal Astronomical Society
- Queen’s University Departments of Physics, Engineering Physics & Astronomy
- CSIRO’s ASKAP radio telescope
- WALLABY Survey
- MeerKAT radio telescope
- University of Manitoba Department of Physics and Astronomy
- Subaru Telescope
- Dark Matter Research
7 comments
anyone here interested in telescopes should check out the MeerKAT in South Africa. it’s supposed to be part of the future steps in this research.
I’m so impressed by the international effort on this one. Scientists from Canada, Australia, South Africa and even more. Just shows what we can discover when we work together.
nathan Deg and Kristine Spekkens are definitely on to something. Keep an eye on them and their work, you guys.
Whoa, polar ring galaxies arent as rare as we thought? That’s kinda huge. I mean, think about what this could mean for understanding dark matter.
The visuals are mind blowing. Imagine the work that went into developing those images. Hats off to Jayanne English.
So, the WALLABY survey is turning out to be a real game changer. How many more discoveries like this are waiting out there?
Exciting but, how sure are they? Whats the next step in confirming this data?