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The Changing View on RR Lyrae Stars

Scientists rethink the age of mysterious RR Lyrae stars.

Bolivia Cuevas-Otahola, Cecilia Mateu, Ivan Cabrera-Ziri, Gustavo Bruzual, Fabiola Hernández-Pérez, Gladis Magris, Holger Baumgardt

― 6 min read


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Table of Contents

RR Lyrae Stars are cool little celestial wonders. They are bright, flickering stars that help astronomers learn about our universe. You can think of them as the reliable streetlights of the vast cosmic highway. They seem to pulse with a regular rhythm, making them perfect for measuring distances in space.

The Old Beliefs

For a long time, scientists thought that RR Lyrae stars only belonged to ancient groups of stars, like those old grandpas sitting in the corner of the cosmic diner, sipping coffee and reminiscing about the good old days. These stars were believed to hang out in older clusters and were seen as markers of older star populations.

But recent findings have started to shake things up. It turns out that some of these stars might be a bit younger than we thought! Imagine if a couple of sprightly teenagers walked into that diner, claiming they belonged with the wise old grandpas. Shocking, right?

The New Quest

So, scientists decided it was time to investigate this cosmic conundrum. They embarked on a mission to find out whether these RR Lyrae stars could actually be younger and belong to intermediate-age groups of stars instead. They figured if they could find RR Lyrae stars hanging out with younger Star Clusters, it might just confirm their new theory.

The Seekers of Truth

To carry out this mission, a group of bright minds utilized some cutting-edge tools. They made use of data from the Gaia Space Mission, which is like having a high-tech camera in the sky snapping pictures of stars and gathering their essential information. They also used data from OGLE, another big star survey that helps astronomers keep track of these flickering lights.

Seeking the Clusters

The scientists set their sights on two regions: the Large and Small Magellanic Clouds, which are like neighboring galaxies that are close enough to visit without needing to pack a suitcase. They looked for RR Lyrae stars near star clusters that were a bit older than 1 billion years.

Using advanced computer models, they sifted through the data and identified a total of 302 RR Lyrae stars that seemed to be hanging out with these clusters. Among them, about 10 stars were likely members of younger groups – a mix of grandpas and sprightly teens!

Understanding the Ages

The researchers dove deeper into the ages of these star populations. They grouped them into categories: ancient (over 10 billion years), young (1 to 2 billion years), and those in between (2 to 8 billion years). They had to be careful to ensure their information was accurate, as they were dealing with stars that have been shining bright for eons.

Using statistical models, they calculated how many RR Lyrae stars should be expected in these various age groups based on their findings.

Hurdles in the Stars

Although they were making progress, it wasn't all smooth sailing. To confirm their suspicions about these intermediate-age RR Lyrae stars, they needed something more concrete than just statistical models. It’s a bit like trying to convince someone that aliens exist – you sort of need a photo, right?

Looking for Confirmation

To solidify their findings, the scientists needed to find RR Lyrae stars in Binary Systems. Binary systems are like the buddy system for stars; they come in pairs, which makes them easier to study. If they could find an RR Lyrae star with a younger star partner, that would be the smoking gun they needed.

However, this task wasn’t easy. They searched but found only a handful of candidates. It was like searching for a needle in a haystack the size of a small galaxy!

The Great Cluster Adventure

Next, they decided to focus on finding RR Lyrae stars in significant clusters. They believed that if they targeted larger clusters, they might have a better chance of encountering these stars. Larger clusters have more stars, increasing the odds of finding RR Lyrae among them.

The Magellanic Clouds were promising locations, as they contained substantial clusters that fit the bill. The scientists scoured through the data and came up with a list of candidates for their search.

The Search Results

After all the hard work, they found several RR Lyrae stars in 10 intermediate-age clusters across the Magellanic Clouds. They were thrilled! Each of these clusters was like a treasure chest, opening up new possibilities for understanding the RR Lyrae stars.

Some of the clusters included familiar names like NGC 339 and NGC 1846, each hosting a few RR Lyrae stars that piqued the researchers’ interest.

Connecting the Dots

The researchers then turned their attention to understanding the rate at which RR Lyrae stars are formed in different age groups. They wanted to know how many of these stars could pop up from various star formation bursts over time.

This required a bit of number crunching and modeling, but the researchers were up for the challenge. They mapped out different age ranges and calculated the production rates of these stars in each category.

The Surprising Findings

Their findings were unusual. They discovered that the rates for RR Lyrae stars in intermediate-age clusters were lower than those in older clusters, confirming their original hypothesis while also leaving room for plenty of new questions. They were like puzzle pieces that didn’t quite fit yet.

The Ongoing Mystery

The researchers realized that even after making these findings, many questions still remained. They acknowledged that the best way to confirm their discoveries would be through further follow-up studies. It would be like continuing a treasure hunt that had only just begun – each new piece of data could shed more light on the importance of these RR Lyrae stars in our understanding of the universe.

Putting It All Together

While many aspects of the research were promising, they knew it wasn't the end. With the precision of upcoming data releases, they hoped that future studies would help confirm these intermediate-age RR Lyrae stars and their peculiar nature.

It felt like they had turned a page in a gripping saga of discovery. The stars continued to hold secrets, and they were just beginning to scratch the surface.

The Takeaway

In conclusion, the quest to study RR Lyrae stars has taken an exciting turn. What was once a simple story about old stars is now a bit more complex. Are RR Lyrae stars really as old as we thought? Or are some of them young enough to still chase after their own cosmic dreams?

Only future studies will tell, and it promises to be a fascinating ride. So, keep your eyes on the sky, and who knows what else we might learn from the twinkling stars above!

Original Source

Title: RR Lyrae Stars in Intermediate-age Magellanic Clusters: Membership Probabilities and Delay Time Distribution

Abstract: Recent works have challenged our canonical view of RR Lyrae (RRL) stars as tracers of exclusively old populations ($\gtrsim10$~Gyr) by proposing a fraction of these stars to be of intermediate ages ($\sim$2-5~Gyr). Since it is currently not possible to infer stellar ages directly for individual RRL stars, our goal in this work is to search for these in association to intermediate-age clusters whose reliable ages can then be safely be attributed to the RRL. We used the Gaia DR3 Specific Object Study and OGLE IV public catalogues to search for RRL stars around stellar clusters older than 1~Gyr in the Large and Small Magellanic Clouds. Modelling membership probabilities based on proper motion and photometric distance we obtained a list of 302 RRL stars associated with Magellanic clusters. Of these, 23 RRL are likely members of 10 intermediate-age clusters: 3 and 7 in the Small and Large Magellanic Clouds, respectively. By modelling the inferred expectation values of the number of RRL stars per cluster, we inferred the delay time distribution of the RRL in three age ranges. For the old population ($>8$~Gyr) we find $2.6^{+0.4}_{-0.3}$ RRL$/10^5 M_\odot$. For the young (1-2 Gyr) and intermediate age (2-8 Gyr) populations we find rates of $0.9^{+0.3}_{-0.2}$ and $0.27^{+0.1}_{-0.09}$ RRL$/10^5 M_\odot$, respectively. While radial velocities are necessary for definitively confirming cluster memberships, the high-probability list of intermediate-age RRL stars presented here offers a promising opportunity for the first direct confirmation of these enigmatic stars.

Authors: Bolivia Cuevas-Otahola, Cecilia Mateu, Ivan Cabrera-Ziri, Gustavo Bruzual, Fabiola Hernández-Pérez, Gladis Magris, Holger Baumgardt

Last Update: 2024-11-19 00:00:00

Language: English

Source URL: https://arxiv.org/abs/2411.12741

Source PDF: https://arxiv.org/pdf/2411.12741

Licence: https://creativecommons.org/licenses/by/4.0/

Changes: This summary was created with assistance from AI and may have inaccuracies. For accurate information, please refer to the original source documents linked here.

Thank you to arxiv for use of its open access interoperability.

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