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Glossary term: 超新星遺跡

Description: 超新星遺跡是超新星爆炸後殘留的結構。它由超新星沖擊產生的熾熱氣體和等離子體組成。在許多超新星遺跡中,恆星超新星爆炸所產生的黑洞或中子星也存在,不過在某些超新星遺跡中,黑洞或中子星已被爆炸的力量拋出。

超新星的爆炸能量會產生沖擊波,沖擊周圍的星際氣體。這種沖擊波將周圍的氣體加熱並電離到極高的溫度(超過一百萬開爾文)。這種高溫氣體會發出各種波長的光,包括 X 射線的重要來源。沖擊還能將粒子加速到很高的速度,使超新星殘骸成為宇宙射線的重要來源。

通過觀察超新星殘骸的膨脹速度,天文學家可以估算出它需要多長時間才能達到目前的大小。這樣,天文學家就能確定超新星爆炸的大致時間。銀河系中的幾顆大型超新星遺跡都是通過這種方法測定的時間,並與天文學家數百年前觀測到的超新星聯繫在一起。

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Term and definition status: The original definition of this term in English have been approved by a research astronomer and a teacher
The translation of this term and its definition is still awaiting approval

This is an automated transliteration of the simplified Chinese translation of this term

The OAE Multilingual Glossary is a project of the IAU Office of Astronomy for Education (OAE) in collaboration with the IAU Office of Astronomy Outreach (OAO). The terms and definitions were chosen, written and reviewed by a collective effort from the OAE, the OAE Centers and Nodes, the OAE National Astronomy Education Coordinators (NAECs) and other volunteers. You can find a full list of credits here. All glossary terms and their definitions are released under a Creative Commons CC BY-4.0 license and should be credited to "IAU OAE".

Related Diagrams


Taurus appears as a y shape with the open end pointing NE. The ecliptic passes WSW to ENE in Taurus’s northern half

Taurus Constellation Map

Caption: The constellation Taurus along with its bright stars and surrounding constellations. Taurus is surrounded by (going clockwise from the top) Perseus, Aries, Cetus, Eridanus, Orion, Gemini and Auriga. Taurus’s brightest star Aldebaran appears in the middle of the constellation. Taurus lies on the ecliptic (shown here as a blue line), this is the path the Sun appears to take across the sky over the course of a year. The Sun is in Taurus from mid May to late June. The other planets of the Solar System can often be found in Taurus. Taurus lies mostly north of the celestial equator with a small part in the celestial southern hemisphere. The whole constellation is visible at some point in the year to whole planet except for the Antarctic and a small region around the North Pole. Taurus is most visible in the evenings in the northern hemisphere winter and southern hemisphere summer. In the eastern part of Taurus we can find the supernova remnant M1 (commonly known as the Crab Nebula), marked here with a green square. In Taurus’s north-east find one of the sky’s most famous open stars clusters M45 (the Pleiades), marked here with a yellow circle. Many of the stars near Aldebaran (but not) Aldebaran are members of another star cluster, the Hyades. However this cluster is close to the solar system so is too dispersed on the sky to have a Messier object designation like the Pleiades has. The y-axis of this diagram is in degrees of declination and with north as up and the x-axis is in hours of right ascension with east to the left. The sizes of the stars marked here relate to the star's apparent magnitude, a measure of its apparent brightness. The larger dots represent brighter stars. The Greek letters mark the brightest stars in the constellation. These are ranked by brightness with the brightest star being labeled alpha, the second brightest beta, etc., although this ordering is not always followed exactly. The dotted boundary lines mark the IAU's boundaries of the constellations and the solid green lines mark one of the common forms used to represent the figures of the constellations. Neither the constellation boundaries, nor the lines joining the stars appear on the sky.
Credit: Adapted by the IAU Office of Astronomy for Education from the original by IAU/Sky & Telescope

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