Mashable 05月07日 17:34
Exceptionally rare radio sources detected in a distant galaxy
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天文学家发现了一个星系团PSZ2 G181.06+48.47周围存在一对罕见的射电遗迹,这些发光的射电能量弧是星系团碰撞后产生的强大冲击波穿过热气体的结果。这对射电遗迹相距约1100万光年,是迄今为止已知的最大距离。研究人员认为,这些射电遗迹是在两个星系团碰撞后,冲击波穿过空间形成的,并迫使粒子发出射电光。此外,科学家们还在遗迹之间发现了一种微弱的光芒,这可能是一种被称为“射电晕”的射电源,它是在剧烈的宇宙碰撞后,翻滚的气体和粒子产生湍流时产生的。

💥星系团碰撞遗迹:天文学家观测到星系团PSZ2 G181.06+48.47周围存在一对射电遗迹,这是由两个星系群碰撞后产生的冲击波所致。

📏超大尺度:这对射电遗迹之间的距离估计为1100万光年,是目前已知的最大间距,远超银河系的尺度。

✨非对称性:虽然这对射电遗迹成对出现,但它们并不完全相同。北部的遗迹更亮且极化,而南部的遗迹形状怪异,能量模式表明它是由更强大的冲击波引起的。

🔭观测设备:研究人员使用印度巨型米波射电望远镜和新墨西哥州甚大阵列发现了这些弧状结构。

🌌潜在发现:未来的平方公里阵列(SKA)可能会发现更多类似的星系团碰撞遗迹。

Astronomers have spotted a pair of exotic features believed to be the aftermath of a colossal cosmic smackdown — not between two galaxies, but two groups of galaxies. 

These glowing arcs of radio energy are known as "radio relics," faint clouds resulting from powerful shockwaves surging through hot gas that fills the space amid a galaxy cluster.

The cluster, PSZ2 G181.06+48.47, is billions of light-years from Earth, but its image is less forgettable than its name. Using the Giant Metrewave Radio Telescope in India and the Very Large Array in New Mexico, a team of researchers spotted the arcs flanking the cluster like giant parentheses. The distance between the punctuation is an estimated 11 million light-years — about 100 times the span of the Milky Way.

That makes their separation a record holder — "the largest known to date," according to a paper published on the discovery in The Astrophysical Journal.

An annotated view of a galaxy cluster reveals a rare pair of radio relics. Credit: Kamlesh Rajpurohit et al / https://iopscience.iop.org/article/10.3847/1538-4357/adbbb9

Galaxies are often part of larger collections of galaxies, held together by gravity, according to NASA. These groups and clusters, containing hundreds to thousands of galactic neighborhoods, serve as building blocks for the larger structures of the universe. Clusters are also composed of scorching gas that reaches millions of degrees as well as dark matter, an invisible material that scientists don't yet fully understand.

The team, led by Kamlesh Rajpurohit, an astronomer at the Harvard & Smithsonian Center for Astrophysics, thinks the newfound radio relics formed when shock fronts sped through space following two clusters wrecking. These waves can force particles to shine in radio light.

Though these two come as a pair, they're not identical twins. The researchers describe the northernmost glow as brighter and polarized, meaning its light is moving in the same direction. Its companion to the south has a stranger ghostly shape and an energy pattern that may mean it was caused by a more powerful shockwave. 

Using an enormous telescope in India and the Very Large Array in New Mexico, pictured above, a team of researchers spotted the arcs flanking the cluster like giant parentheses. Credit: Bettymaya Foott / NRAO / AUI / NSF

The relics suggest the entire cluster is in the final throes of a merger set in motion a billion years before.

In the past, astronomers have dubbed clusters fun nicknames based on the shapes of their relics, such as the Toothbrush Cluster. Perhaps in the future this one will leave behind its numerical moniker for something a bit snazzier, like the Eyebrows Cluster or the Air Quotes Cluster. Until that time, you can call it Planck cluster G181+48 for short, Rajpurohit said.

Scientists discovered one other curiosity between the relics: a faint glow at the center of the cluster. This could be a so-called "radio halo," another kind of radio source that emerges when churning gas and particles create turbulence after a violent cosmic crash.

Astronomers have previously detected less than 30 such clusters with relic pairs. But the upcoming Square Kilometre Array being built in South Africa and Australia could be a "game changer," according to the paper's authors. 

"There could potentially be many more awaiting discovery in the era of large radio surveys," they said.

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星系团 射电遗迹 宇宙碰撞 天文学 冲击波
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