File:G19 xray.tif
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[edit]DescriptionG19 xray.tif |
English: G1.9+0.3 is the remains of the most recent supernova, in Earth's time frame, known to have occurred in the Milky Way. If gas and dust had not heavily obscured it, the explosion would have been visible from Earth just over a century ago. A new long Chandra observation - equivalent to over 11 days of time - reveals new details about the explosion.
Fast Facts for G1.9+0.3: Credit X-ray (NASA/CXC/NCSU/K.Borkowski et al.) Release Date June 26, 2013 Scale Image is 8 arcmin across (About 60 light years) Category Supernovas & Supernova Remnants Coordinates (J2000) RA 17h 48m 45s - Dec -27° 10' 00" Constellation Sagittarius Observation Date 15 pointings between Feb 2007 and Jul 2011 Observation Time 362 hours (15 days 2 hours) Obs. ID 6708, 8521, 10111, 10112, 10928, 10930, 12689-95, 13407, 13509 Instrument ACIS References Borkowski, K, et al, 2013, ApJ Letters (Submitted); arXiv:1305.7399 Color Code X-ray (Red, Green, Blue). |
Date | |
Source | http://chandra.harvard.edu/photo/2013/g19/ http://chandra.harvard.edu/photo/2013/g19/g19_xray.tif |
Author | NASA/CXC/NCSU/K.Borkowski et al. |
Permission (Reusing this file) |
See Category:Chandra_images |
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[edit]Public domainPublic domainfalsefalse |
This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.) | ||
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current | 17:30, 3 January 2014 | 1,500 × 1,280 (804 KB) | Fabian RRRR (talk | contribs) | crop | |
17:25, 3 January 2014 | 3,600 × 3,600 (984 KB) | Fabian RRRR (talk | contribs) | =={{int:filedesc}}== {{Information |description={{en|1=G1.9+0.3 is the remains of the most recent supernova, in Earth's time frame, known to have occurred in the Milky Way. If gas and dust had not heavily obscured it, the explosion would have been visi... |
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Image title | A new Chandra observation is providing important details about the most recent supernova known to have exploded in the Milky Way. The explosion would have been visible from Earth a little more than a hundred years ago if it had not been heavily obscured by dust and gas. G1.9+0.3 was most likely created when a white dwarf star underwent a thermonuclear detonation and was destroyed - either after merging with another white dwarf or by pulling too much material from an orbiting companion star. The Chandra data show that most of the X-ray emission is "synchrotron radiation," produced by extremely energetic electrons accelerated in the rapidly expanding blast wave of the supernova. The new X-ray study also reveals that the explosion that created G1.9+0.3 was asymmetrical and unusually energetic. |
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Height | 1,280 px |
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Compression scheme | LZW |
Pixel composition | RGB |
Orientation | Normal |
Number of components | 3 |
Number of rows per strip | 64 |
Horizontal resolution | 300 dpi |
Vertical resolution | 300 dpi |
Data arrangement | chunky format |
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