What is the translation of " IA型超新星 " in English?

type ia supernovae
ia 型 超 新星
在 ia型 超 新星
type la supernova
ia 型 超 新星
type ia supernova
ia 型 超 新星
在 ia型 超 新星
type ia supernovas
ia 型 超 新星
在 ia型 超 新星
type la supernovae
ia 型 超 新星
sne ia

Examples of using Ia型超新星 in Chinese and their translations into English

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Ia型超新星能否作为标准烛光也因之有了疑问。
Type La supernova can also be used as standard candles.
观测Ia型超新星发现存在暗能量.
Observations of the Type la supernovae revealed the existence of dark energy.
然而还有许多困难困扰着对Ia型超新星的研究。
However, there is an ongoing controversy about Type La supernovas.
然而还有许多困难困扰着对Ia型超新星的研究。
There is also much research on type La supernovae.
先前对至少两个Ia型超新星的观测在爆炸后几个月检测到了发光碎片。
Prior observations of at least two Type Ia supernovae detected glowing debris months after the explosion.
Ia型超新星,也称为“标准蜡烛”,以相似的方式工作,因为它们始终以大约相同的光量发光。
He analyzes Type Ia supernovae, called“standardizable candles,” because they all have essentially the same brightness.
SN2014J,一颗Ia型超新星,是2014年1月21日在这个星系内发现的超新星。
SN 2014J, a type La supernova, was discovered in the galaxy on January 21, 2014.
有少量低红移Ia型超新星,曾经用几架望远镜同时观测过,它们提供了一种途径,可以对它们的相对校准提供评估。
A few low-z SNe Ia have been observed contemporaneously with several telescopes which provides a way to assess their relative calibration.
沙特说:“Ia型超新星是了解整个宇宙如何膨胀和增长的关键部分。
Type la supernova are a critical part of understanding how the entire universe expands and grows.
根据格雷厄姆的说法,Ia型超新星已被用于宇宙学研究,因为它们的一致光度使它们成为理想的“宇宙灯塔”。
Astronomers have used Type Ia supernovae for cosmological studies because their consistent luminosity makes them ideal“cosmic lighthouses,” Graham says.
常见的一类爆炸的恒星(被称作Ia型超新星)有着相当均一的亮度,后者对宇宙学研究颇为有用。
A common group of exploding stars, known as Type Ia supernovae, have a fairly uniform brightness that makes them useful for cosmology.
SN2014J,一颗Ia型超新星,是2014年1月21日在这个星系内发现的超新星。
SN 2014J, a Type La supernova, was observed in the galaxy on 21 January 2014.
Ia型超新星的发现由哈勃太空望远镜的Z1:过去的减速和暗能量演化的限制证据.
Type Ia Supernova Discoveries at zgt; 1 from the Hubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution.
SN2014J被归类为Ia型超新星,并且是至少四十年来最接近的这种爆发。
SN 2014J is classified as a Type Ia supernova and is the closest such blast in at least four decades.
天文学家使用这些所谓的Ia型超新星作为宇宙距离标记来测量宇宙的膨胀。
Astronomers use these so-called Type Ia supernovas as cosmic distance markers to measure the expansion of the Universe.
G299可能是这种“不寻常”Ia型超新星的一个例子。
G299 could be an example of such an“unusual” Type La supernova.
Ia型超新星具有特征性的光度曲线,在爆炸发生后它的光度是时间的函数。
Type Ia supernovae have a characteristic light curve, their graph of luminosity as a function of time after the explosion.
Ia型超新星,也称为“标准蜡烛”,以相似的方式工作,因为它们始终以大约相同的光量发光。
Type Ia supernovae, also referred to as“standard candles,” work in a similar way because they consistently shine with about the same amount of light.
Ia型超新星需要完全破坏一颗白矮星,这是由太阳等恒星产生的紧凑残余物。
Type Ia supernovas entail the total destruction of a white dwarf, a compact remnant produced by stars like the Sun.
SN2014J,一颗Ia型超新星,是2014年1月21日在这个星系内发现的超新星。
SN 2014J, a Type Ia supernova, was observed in the galaxy on 21 January 2014, see 2014 supernova..
Ia型超新星在帮助天文学家了解宇宙方面发挥着至关重要的作用。
Type La supernovae play a crucial role in helping astronomers understand the universe.
它与通常的Ia型超新星不同,于先前发现的几个奇特Ia型超新星也不同,例如SN1991T和SN1991bg。
It behaved differently from normal type Ia supernovae,and differently from several other previously observed peculiar type Ia supernovae including SN 1991T and SN 1991bg.
天文学家在附近含有Ia型超新星的星系中寻找造父变星,以便他们可以比较这两种恒星的真实亮度。
Astronomers search for Cepheid variables in nearby galaxies containing a Type Ia supernova so they can compare the true brightness of both types of stars.
一组科学家包括来自芝加哥大学的学者,似乎已经发现了第一张来自Ia型超新星的x射线。
A team of scientists, including scholars from the University of Chicago,appear to have found the first X-rays coming from type Ia supernovas.
科学家估计,我们的银河系每1千年就有3个Ia型超新星
In our Galaxy, scientists estimate that there are three Type La supernovae every thousand years.
钱德拉数据显示的模式表明,这种Ia型超新星可能产生非常不平衡的爆炸。
The patterns seen in the Chandra data suggest that a verylopsided explosion may have produced this Type Ia supernova.
而当前对哈勃常数的最精确测量来自于Ia型超新星
The most accuratedeterminations of the Hubble parameter H0 come from Type La supernovae.
其次,ASASSN-18tb喷射的氢气量明显少于其他Ia型超新星周围的氢气量。
Second, the amount of hydrogen ejected by ASASSN-18tb issignificantly less than that seen surrounding those other Type Ia supernovae.
这里,我们报告了Ia型超新星的光谱的差异与它们的诞生地的环境有关。
Here, we report that the spectral diversity of SNe Ia is tied to their birthplace environments.
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