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The Mysterious Dance of V338 Boo

Astronomers observe the strange pulsation patterns of RR Lyrae star V338 Boo.

Kenneth Carrell, Ronald Wilhelm, Andrew Tom, Horace Smith, Adam Popowicz, Gary Hug, Stephen M. Brincat, Fabio Salvaggio, Keith Nakonechny, Darrell Lee, Teofilo Arranz Heras, Tony Vale, Davide Mortari, Andre Steenkamp, Ralph Rogge, Jacek Checinski

― 6 min read


V338 Boo: A Star’s V338 Boo: A Star’s Surprise Show inquiries. patterns, sparking new astronomical V338 Boo exhibits strange pulsation
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Have you ever tried to catch a magician in the middle of a trick? Well, astronomers have been trying to catch a star doing something pretty magical too! They have their eyes on a star called V338 Boo, which has been throwing them a few curveballs. This star is part of a special group known as RR Lyrae Stars. These stars are known for their twinkling personalities, kind of like a dramatic friend who always has a surprise up their sleeve.

What’s the Buzz About V338 Boo?

V338 Boo is not just any star; it’s a double-mode RR Lyrae star, which means it can pulsate in two different ways at the same time. Imagine you can dance the cha-cha and the tango simultaneously-pretty impressive, right? Well, V338 Boo was recently observed behaving rather strangely.

In 2022, astronomers decided to take a second look at V338 Boo using a satellite called TESS. It’s like giving your friend a second chance to impress you after they flubbed a magic trick. During the observation, something unexpected happened: one of V338 Boo's Pulsation Modes took a break, almost as if it got stage fright!

The Great Pulsation Disappearance

During the TESS observations, researchers noticed that the first overtone pulsation mode vanished completely. Picture a drama queen who storms off the stage during a performance-except in this case, the star was actually having an off day! But wait, there’s a plot twist! Right after a little break, this pulsing mode decided to rejoin the party and even became the star of the show!

After the TESS observations wrapped up, the AAVSO, a group that loves watching variable stars, took over and found that the first overtone mode didn’t just come back; it became the most prominent pulsation mode. So, it seems like this star really enjoys being the center of attention.

A Sneak Peek into the Past

Let’s rewind a bit to see how we got here. Back in the late 1800s, an astronomer named Williamina Fleming discovered a talented variable star in the constellation Lyra, which we now call RR Lyrae. This star was the star of its own show, becoming the role model for other stars in the RR Lyrae family.

Over the years, scientists classified these stars into various types, and V338 Boo fell into the category of RRd stars. These are the stars that can perform in both their fundamental and first overtone modes. It’s as if they’re pretending to juggle while also dancing.

But every magician has their secrets. Early observers noticed some RR Lyrae stars had light variations that didn’t add up, like missing a trick in a magic act. It was later found that these changes might be due to a phenomenon called mode mixing, where the star’s pulsation modes dance with each other in unexpected ways.

The Blazhko Effect: A Star's Mystery

Now, here’s where things get even more interesting. Some RR Lyrae stars experience an odd behavior known as the Blazhko effect, a periodic fluctuation in brightness. Imagine your friend who can’t decide whether to sing the chorus or stick to the verse of a song-it’s a bit confusing!

This Blazhko effect has puzzled astronomers for ages, and V338 Boo has become a key player in trying to figure out this star-studded mystery. V338 Boo is not alone; there are other stars in the RR Lyrae family that might hold the secret to the Blazhko effect, just waiting for their moment in the spotlight.

V338 Boo’s Journey Continues

Let’s give a round of applause to V338 Boo for putting on such an intriguing show! This star has been in the spotlight for almost two decades, and each performance brings new surprises. Researchers discovered that the period ratio of its pulsations is just right for an RRd star. It’s like finding out that the magician actually knows a lot more than they let on!

In previous observations, it was noted that the amplitude of the Fundamental Mode was larger than that of the first overtone mode. However, a few years later, this relationship changed, leaving researchers scratching their heads. Imagine attending a magic show where the magician suddenly starts performing a different set of tricks!

The Latest Observations

Fast forward to 2022-TESS decided to give V338 Boo another round of applause. The observations took place in early spring, and scientists were eager to see if the star would keep up its performance or take another unexpected break.

When the TESS team analyzed the data, they discovered significant changes in the amplitudes of both pulsation modes during the observations. The fundamental mode rose to prominence like a star taking center stage, while the first overtone mode seemed to fade. In fact, it completely disappeared during a brief window.

What Did We Learn?

Let’s break it down. V338 Boo showcased some thrilling and bizarre behavior-losing its first overtone mode for a short time, then immediately bouncing back. It’s like the star had a moment of hesitation before returning with a dazzling pirouette. Astronomers saw that this wasn’t just a one-time stunt; it seemed to follow a pattern.

With the follow-up observations from the AAVSO, it became clear that the first overtone mode grew dominant once again, suggesting periodic behavior. It’s like V338 Boo found a rhythm and decided to stick with it!

Questions That Need Answers

While the show was impressive, it also raised a ton of questions. Could this mode-switching behavior be a sign of some deeper cosmic secrets? Other stars have exhibited this “switcheroo” before, prompting scientists to wonder if it’s common among all RR Lyrae stars.

V338 Boo has opened the door to the idea that some stars might also experience periodic changes that observers mistook for a complete transformation. Imagine getting confused by a magician who suddenly pulls a rabbit out of a hat instead of a scarf!

The Blazhko Effect and V338 Boo

The nagging question remains: Does the behavior of V338 Boo relate to the Blazhko effect? Since V338 Boo showcases periodic changes in both modes, some scientists are starting to think it might still be under the influence of the Blazhko magic.

Comparing it to other RR Lyrae stars that show some kind of modulation is vital. However, there are differences that make V338 Boo a unique puzzle. For example, many other stars with similar effect show unusual amplitude changes, while V338 Boo’s modes often move in sync.

Concluding Thoughts

In the end, researchers have their hands full with V338 Boo and its behavior. The star is more than just another celestial object; it’s a delightful enigma, a dazzling performer in the night sky that keeps giving us surprises.

As astronomers keep observing this star, they hope to unveil even more of its mysteries. After all, every good magician needs a great audience, and for V338 Boo, the cosmic crowd is paying close attention, ready to applaud its next stunning act!

Original Source

Title: Caught in the Act: Observations of the Double-mode RR Lyrae V338 Boo During the Disappearance of a Pulsation Mode

Abstract: New results on the behavior of the double-mode RR Lyrae V338 Boo are presented. The Transiting Exoplanet Survey Satellite (TESS) observed this star again in 2022, and an observing campaign of the American Association of Variable Star Observers (AAVSO) was completed after the TESS observations as a follow-up. We find that the first overtone pulsation mode in this star completely disappears during the TESS observing window. This mode reappears at the end of the TESS observations, and the AAVSO observing campaign shows that in the months that followed, the first overtone mode was not only present, but was the dominant mode of pulsation. This star, and potentially others like it, could hold the key to finally solving the mystery of the Blazhko effect in RR Lyrae.

Authors: Kenneth Carrell, Ronald Wilhelm, Andrew Tom, Horace Smith, Adam Popowicz, Gary Hug, Stephen M. Brincat, Fabio Salvaggio, Keith Nakonechny, Darrell Lee, Teofilo Arranz Heras, Tony Vale, Davide Mortari, Andre Steenkamp, Ralph Rogge, Jacek Checinski

Last Update: 2024-11-14 00:00:00

Language: English

Source URL: https://arxiv.org/abs/2411.09739

Source PDF: https://arxiv.org/pdf/2411.09739

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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