NGC 1929 en la nube de magallanes, una galaxia satélite de nuestra vía lactea a 160 mil años luz.

NGC 1929 en la nube de magallanes, una galaxia satélite de nuestra vía lactea a 160 mil años luz.

Nebula Images: http://ift.tt/20imGKa Astronomy articles:...  Nebula Images: http://ift.tt/20imGKa  Astronomy articles: http://ift.tt/1K6mRR4  nebula nebulae astronomy space nasa hubble telescope kepler telescope stars apod http://ift.tt/2hWmdjy

Nebula Images: http://ift.tt/20imGKa Astronomy articles:... Nebula Images: http://ift.tt/20imGKa Astronomy articles: http://ift.tt/1K6mRR4 nebula nebulae astronomy space nasa hubble telescope kepler telescope stars apod http://ift.tt/2hWmdjy

‘Hand of God,’ this object is called a pulsar wind nebula. It's powered by the leftover, dense core of a star that blew up in a SN explosion. The stellar corpse, called PSR B1509-58, is a pulsar. NASA's NuSTAR spacecraft has imaged the struc-ture in high-energy X-rays for the 1st time: blue:: lower energy X-Ray light previously detected by Chandra: green & red | NASA:

‘Hand of God,’ this object is called a pulsar wind nebula. It's powered by the leftover, dense core of a star that blew up in a SN explosion. The stellar corpse, called PSR B1509-58, is a pulsar. NASA's NuSTAR spacecraft has imaged the struc-ture in high-energy X-rays for the 1st time: blue:: lower energy X-Ray light previously detected by Chandra: green & red | NASA:

The cluster is surrounded by clouds of interstellar gas and dust—the raw material for new star formation. The nebula, located 20,000 light-years away in the constellation Carina, contains a central cluster of huge, hot stars, called NGC 3603.  CREDIT: NASA, ESA, R., F. Paresce, E. Young, the WFC3 Science Oversight Committee, and the Hubble Heritage Team

The cluster is surrounded by clouds of interstellar gas and dust—the raw material for new star formation. The nebula, located 20,000 light-years away in the constellation Carina, contains a central cluster of huge, hot stars, called NGC 3603. CREDIT: NASA, ESA, R., F. Paresce, E. Young, the WFC3 Science Oversight Committee, and the Hubble Heritage Team

#NGC474 is an elliptical galaxy in the constellation Pisces. This large galaxy is known to possess tidal tails, although their origins remain unknown. These tidal tails may be related to debris left over from absorbing numerous small galaxies in the past billion years.

#NGC474 is an elliptical galaxy in the constellation Pisces. This large galaxy is known to possess tidal tails, although their origins remain unknown. These tidal tails may be related to debris left over from absorbing numerous small galaxies in the past billion years.

See Explanation.  Clicking on the picture will download  the highest resolution version available.

See Explanation. Clicking on the picture will download the highest resolution version available.

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