NASA - Observing our universe in different kinds of light 🌌Each of these images combines data from our @NASAChandraXray observat|图文|广告营销案例【ADGuider广告指南】

NASA-在不同种类的光中观察我们的宇宙这些图像中的每一个都结合了来自我们的 @ NASAChandraXray观察站的数据

案例简介：用不同的光观察我们的宇宙这些图像中的每一个都将我们的 @ NASAChandraXray天文台的数据与其他任务的数据相结合。这种 “多波长” 的天文学方法有助于我们更全面地了解太空中的物体。1.这个螺旋星云图像包含来自我们的Spitzer太空望远镜的红外数据 (绿色和红色)，来自我们的 @ NASAHubble太空望远镜的光学光 (橙色和蓝色)，来自我们的银河系演化探测器的紫外线 (青色)，钱德拉的x射线 (显示为白色) 显示了在星云中心形成的白矮星。图像约为四光年。信用: x射线: NASA/CXC; 紫外线: NASA/jpl-caltech/SSC; 光学: NASA/STScI(M.迈克斯纳)/欧洲航天局/NRAO(T.A.校长); 红外线: NASA/jpl-caltech/K。Su)2。车轮星系类似于牛眼，这是适当的，因为它的出现部分是由于穿过该物体中间的较小星系。来自钱德拉 (紫色) 的x射线显示，最初由车轮星系承载的扰动热气体被碰撞拖了超过150,000光年。来自哈勃的光学数据 (红色，绿色和蓝色) 显示了这次碰撞可能引发恒星形成的地方。来源: x射线: NASA/CXC; 光学: NASA/STScI)3。Eta Carinae是一个挥发性系统，包含两个彼此紧密围绕的大质量恒星。此图像有三种类型的光: 来自哈勃的光学数据 (显示为白色)，来自哈勃的紫外线 (青色) 和来自钱德拉的x射线 (显示为紫色发射)。来源: NASA/CXC; 紫外线/光学: NASA/STScI; 组合图像: NASA/ESA/N.史密斯 (亚利桑那大学)，J。莫里斯 (BoldlyGo Instituts) 和A.Pagan)4。大麦哲伦星云中的超新星1987A (SN 1987A) 是几个世纪以来最亮的超新星爆炸之一。钱德拉数据 (蓝色) 显示了超新星休克波与周围物质相互作用的位置，距离原始爆炸点约4光年。来自哈勃 (橙色和红色) 的光学数据也显示了环中这种相互作用的证据。信用: 无线电: ALMA (ESO/NAOJ/NRAO)，P。Cigan和R.独立; NRAO/

NASA-在不同种类的光中观察我们的宇宙这些图像中的每一个都结合了来自我们的 @ NASAChandraXray观察站的数据

案例简介：Observing our universe in different kinds of light 🌌Each of these images combines data from our @NASAChandraXray observatory with data from other missions. This "multiwavelength" approach to astronomy helps us get a more complete understanding of objects in space. 1. This Helix Nebula image contains infrared data from our Spitzer Space Telescope (green and red), optical light from our @NASAHubble Space Telescope (orange and blue), ultraviolet from ours Galaxy Evolution Explorer (cyan), and Chandra's X-rays (appearing as white) showing the white dwarf star that formed in the center of the nebula. The image is about four light years across.Credit: X-ray: NASA/CXC; Ultraviolet: NASA/JPL-Caltech/SSC; Optical: NASA/STScI(M. Meixner)/ESA/NRAO(T.A. Rector); Infrared: NASA/JPL-Caltech/K. Su)2. The Cartwheel Galaxy resembles a bull's eye, which is appropriate because its appearance is partly due to a smaller galaxy that passed through the middle of this object. X-rays from Chandra (purple) show disturbed hot gas initially hosted by the Cartwheel galaxy being dragged over more than 150,000 light years by the collision. Optical data from Hubble (red, green, and blue) show where this collision may have triggered the star formation.Credit: X-ray: NASA/CXC; Optical: NASA/STScI)3. Eta Carinae is a volatile system containing two massive stars that closely orbit each other. This image has three types of light: optical data from Hubble (appearing as white), ultraviolet (cyan) from Hubble, and X-rays from Chandra (appearing as purple emission).Credit: NASA/CXC; Ultraviolet/Optical: NASA/STScI; Combined Image: NASA/ESA/N. Smith (University of Arizona), J. Morese (BoldlyGo Instituts) and A. Pagan)4. Supernova 1987A (SN 1987A) in the Large Magellanic Cloud was one of the brightest supernova explosions in centuries. The Chandra data (blue) show the location of the supernova's shock wave interacting with the surrounding material about four light years from the original explosion point. Optical data from Hubble (orange and red) also shows evidence for this interaction in the ring.Credit: Radio: ALMA (ESO/NAOJ/NRAO), P. Cigan and R. Indebetouw; NRAO/