「すごい」 – 初めてキャッツアイ星雲を 3D で見る

天文学者は、キャッツアイ星雲でほぼ完全な対称性を持つリングを発見します

研究者は、キャッツアイ星雲の最初のコンピューター生成 3D モデルを構築し、星雲の外殻の周りに対称的なリングのペアを明らかにしました。 リングの対称性は、それらが星雲の中心星から発生したジェット気流によって形成されたことを示しています。 これは、星雲の中心にある連星の強力な証拠を提供します。 この研究は最近ジャーナルに掲載されました 王立天文学会の月例通知 ライアン・クレアモントが率いていました。

惑星状星雲は、瀕死の星がガスの外層を放出するときに形成され、惑星状星雲の特徴である色とりどりの殻のような構造を作り出します。 NGC 6543、またはキャッツアイ星雲は、知られている最も複雑な惑星状星雲の 1 つです。 地球からの距離は 3,000 光年強で、りゅう座に見えます。 キャッツアイ星雲はまた、[{” attribute=””>Hubble Space Telescope, exhibiting a complicated structure of knots, spherical shells, and arc-like filaments.

A side-by-side comparison of the three-dimensional model of the Cat’s Eye Nebula created by Clairmont and the Cat’s Eye Nebula as photographed by the Hubble Space Telescope. Ryan Clairmont (left), NASA, ESA, HEIC, and The Hubble Heritage Team (STScI/AURA) (right) (CC BY-NC-SA 4.0).

The nebula’s mysterious structure confounded astrophysicists because it could not be explained by previously accepted theories for planetary nebula formation. More recent research showed that precessing jets were potential shaping mechanisms in complex planetary nebulae such as NGC 6543, but lacked a detailed model.

Clairmont, an astronomy enthusiast, decided to try to establish the detailed 3D structure of the Cat’s Eye to find out more about the potential mechanism that gave it its intricate shape. To do this, he sought out the help of Dr. Wolfgang Steffen of The National Autonomous University of Mexico and Nico Koning from the University of Calgary, who developed SHAPE, 3D astrophysical modeling software particularly suitable for planetary nebulae.

The researchers used spectral data from the San Pedro Martir National Observatory in Mexico to reconstruct the nebula’s three-dimensional structure’s three-dimensional structure. These provide detailed information on the internal motion of material in the nebula. Together with these data and images from the Hubble Space Telescope, Clairmont constructed a novel 3D model, establishing that rings of high-density gas were wrapped around the outer shell of the Cat’s Eye. Surprisingly, the rings are almost perfectly symmetric to each other, suggesting they were formed by a jet – a stream of high-density gas ejected in opposite directions from the nebula’s central star.

The jet exhibited precession, similar to the wobbling motion of a spinning top. As the jet wobbled, or precessed, it outlined a circle, creating the rings around the Cat’s Eye. However, the data indicates the rings are only partial, meaning the precessing jet never completed a full 360-degree rotation, and that the emergence of the jets was only a short-lived phenomenon. The duration of outflows is an important piece of information for the theory of planetary nebulae. Since only binary stars can power a precessing jet in a planetary nebula, the team’s findings are strong evidence that a system of this type exists at the center of the Cat’s Eye.

As the angle and direction of the jet changed over time, it likely formed all of the features seen in the Cat’s Eye, including the jets and knots. Using the three-dimensional model, the researchers were able to calculate the tilt and opening angle of the precessing jet based on the orientation of the rings.

Ryan Clairmont, the lead author of the paper and now a prospective undergraduate at Stanford University stated, “When I first saw the Cat’s Eye Nebula, it was astonishing. It had a beautiful, perfectly symmetric structure. I was even more surprised that its 3D structure was not fully understood.”

He continued, “It was very rewarding to be able to do astrophysical research of my own that actually has an impact in the field. Precessing jets in planetary nebulae are relatively rare, so it’s important to understand how they contribute to the shaping of more complex systems like the Cat’s Eye. Ultimately, understanding how they form provides insight into the eventual fate of our Sun, which will itself one day become a planetary nebula.”

Reference: “Morphokinematic modelling of the point-symmetric Cat’s Eye, NGC 6543: Ring-like remnants of a precessing jet” by Ryan Clairmont, Wolfgang Steffen and Nico Koning, 15 September 2022, Monthly Notices of the Royal Astronomical Society.
DOI: 10.1093/mnras/stac2375