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NASA-我们发现磁场非常有吸引力🧲该图像显示了超新星残骸SN 1006。它结合了我们成像X的数据-
案例简介:我们发现磁场非常有吸引力此图显示了超新星遗迹SN 1006。它结合了来自我们的成像x射线偏振测量浏览器 (IXPE) 和 @ nasachandraxray的数据。红色,绿色和蓝色元素反射低,中和高能x射线。测量x射线光的偏振的IXPE数据以紫色显示在左上角,加上代表残余磁场向外运动的线。研究人员说,结果表明磁场与残余高能粒子流出之间存在联系。以更高的细节和准确性绘制这些超新星残留物的磁场结构,使我们能够更好地理解驱动这些粒子加速的过程。SN 1006在狼疮星座中距离地球约6,500光年。它是发生在两个白矮星合并或白矮星从伴星中拉出过多质量时发生的大规模爆炸的遗骸,这被认为是历史上记录的最亮的恒星事件。爆炸恒星的碎片就像一个斑驳的红球,在柔和的恒星背景下搅动着火焰。超新星遗迹似乎被薄纱蓝色和白色环包围,在我们的右下和左上最突出。这种结构与其他圆形超新星遗迹明显不同。在左上角,SN 1006的标记部分以蓝色圆圈突出显示。在这个圆圈内,只显示了超新星遗迹的外环,没有显示内部搅动的斑驳的红色恒星物质。这个环是超新星膨胀爆炸波的一部分,钱德拉和IXPE都在x射线光中观察到。磁场线在圆圈中显示为尖刺的白线,大部分指向上方并指向左侧。Spitzer太空望远镜在红外光下捕获了恒星的背景。图片来源: x射线: NASA/CXC/SAO (Chandra); NASA/MSFC/南京大学/P。Zhou et al. (IXPE); IR: NASA/JPL/Caltech/Spitzer; Image Processing: NASA/CXC/SAO/J.Schmidt # NASA # Space # Supernova
NASA-我们发现磁场非常有吸引力🧲该图像显示了超新星残骸SN 1006。它结合了我们成像X的数据-
案例简介:We find magnetic fields very attractive 🧲This image shows supernova remnant SN 1006. It combines data from our Imaging X-ray Polarimetry Explorer (IXPE) and @nasachandraxray. The red, green, and blue elements reflect low, medium, and high energy X-rays. The IXPE data, which measure the polarization of the X-ray light, is show in purple in the upper left corner, with the addition of lines representing the outward movement of the remnant’s magnetic field.Researchers say the results show a connection between the magnetic fields and the remnants high-energy particle outflow. Mapping these magnetic field structures of supernova remnants at higher energies with enhanced detail and accuracy enables us to better understand the processes driving the acceleration of these particles.SN 1006 is about 6,500 light-years from Earth in the Lupus constellation. It is the remains of a massive explosion which occurred with when two white dwarfs merged or when a white dwarf pulled too much mass from a companion star – creating what is thought to be the brightest stellar event recorded in history.Image description: The debris from an exploded star resembles a mottled red ball of churning fire against a softer backdrop of stars. The supernova remnant appears to be encircled by a gauzy blue and white ring that is most prominent at our lower right and upper left. This structure is markedly different from other rounded supernova remnants. At the upper lefthand corner, a labeled section of SN 1006 is highlighted in a blue-tinted circle. Within this circle, only the outer ring of the supernova remnant is shown, not the mottled red stellar material churning inside. This ring is part of the supernova's expanding blast wave, which has been observed in X-ray light by both Chandra and IXPE. Magnetic field lines are illustrated in the circle as spiky, white lines, pointing mostly upwards and toward the left. The backdrop of stars was captured in infrared light by the Spitzer Space Telescope.Credit: X-ray: NASA/CXC/SAO (Chandra); NASA/MSFC/Nanjing Univ./P. Zhou et al. (IXPE); IR: NASA/JPL/Caltech/Spitzer; Image Processing: NASA/CXC/SAO/J.Schmidt #NASA #Space #Supernova
NASA - We find magnetic fields very attractive 🧲This image shows supernova remnant SN 1006. It combines data from our Imaging X-
案例简介:我们发现磁场非常有吸引力此图显示了超新星遗迹SN 1006。它结合了来自我们的成像x射线偏振测量浏览器 (IXPE) 和 @ nasachandraxray的数据。红色,绿色和蓝色元素反射低,中和高能x射线。测量x射线光的偏振的IXPE数据以紫色显示在左上角,加上代表残余磁场向外运动的线。研究人员说,结果表明磁场与残余高能粒子流出之间存在联系。以更高的细节和准确性绘制这些超新星残留物的磁场结构,使我们能够更好地理解驱动这些粒子加速的过程。SN 1006在狼疮星座中距离地球约6,500光年。它是发生在两个白矮星合并或白矮星从伴星中拉出过多质量时发生的大规模爆炸的遗骸,这被认为是历史上记录的最亮的恒星事件。爆炸恒星的碎片就像一个斑驳的红球,在柔和的恒星背景下搅动着火焰。超新星遗迹似乎被薄纱蓝色和白色环包围,在我们的右下和左上最突出。这种结构与其他圆形超新星遗迹明显不同。在左上角,SN 1006的标记部分以蓝色圆圈突出显示。在这个圆圈内,只显示了超新星遗迹的外环,没有显示内部搅动的斑驳的红色恒星物质。这个环是超新星膨胀爆炸波的一部分,钱德拉和IXPE都在x射线光中观察到。磁场线在圆圈中显示为尖刺的白线,大部分指向上方并指向左侧。Spitzer太空望远镜在红外光下捕获了恒星的背景。图片来源: x射线: NASA/CXC/SAO (Chandra); NASA/MSFC/南京大学/P。Zhou et al. (IXPE); IR: NASA/JPL/Caltech/Spitzer; Image Processing: NASA/CXC/SAO/J.Schmidt # NASA # Space # Supernova
NASA - We find magnetic fields very attractive 🧲This image shows supernova remnant SN 1006. It combines data from our Imaging X-
案例简介:We find magnetic fields very attractive 🧲This image shows supernova remnant SN 1006. It combines data from our Imaging X-ray Polarimetry Explorer (IXPE) and @nasachandraxray. The red, green, and blue elements reflect low, medium, and high energy X-rays. The IXPE data, which measure the polarization of the X-ray light, is show in purple in the upper left corner, with the addition of lines representing the outward movement of the remnant’s magnetic field.Researchers say the results show a connection between the magnetic fields and the remnants high-energy particle outflow. Mapping these magnetic field structures of supernova remnants at higher energies with enhanced detail and accuracy enables us to better understand the processes driving the acceleration of these particles.SN 1006 is about 6,500 light-years from Earth in the Lupus constellation. It is the remains of a massive explosion which occurred with when two white dwarfs merged or when a white dwarf pulled too much mass from a companion star – creating what is thought to be the brightest stellar event recorded in history.Image description: The debris from an exploded star resembles a mottled red ball of churning fire against a softer backdrop of stars. The supernova remnant appears to be encircled by a gauzy blue and white ring that is most prominent at our lower right and upper left. This structure is markedly different from other rounded supernova remnants. At the upper lefthand corner, a labeled section of SN 1006 is highlighted in a blue-tinted circle. Within this circle, only the outer ring of the supernova remnant is shown, not the mottled red stellar material churning inside. This ring is part of the supernova's expanding blast wave, which has been observed in X-ray light by both Chandra and IXPE. Magnetic field lines are illustrated in the circle as spiky, white lines, pointing mostly upwards and toward the left. The backdrop of stars was captured in infrared light by the Spitzer Space Telescope.Credit: X-ray: NASA/CXC/SAO (Chandra); NASA/MSFC/Nanjing Univ./P. Zhou et al. (IXPE); IR: NASA/JPL/Caltech/Spitzer; Image Processing: NASA/CXC/SAO/J.Schmidt #NASA #Space #Supernova
NASA-我们发现磁场非常有吸引力🧲该图像显示了超新星残骸SN 1006。它结合了我们成像X的数据-
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NASA - We find magnetic fields very attractive 🧲This image shows supernova remnant SN 1006. It combines data from our Imaging X-
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