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NGC 1672 - JWST - Chandra - Hubble - Magnification and reconstruction via AI.
Reconstruction using our artificial intelligence model from an image provided by Chandra X-ray Observatory about NGC 1672.
NGC 1672 is a spiral galaxy, but one that astronomers categorize as a “barred” spiral. In regions close to their centers, the arms of barred spiral galaxies are mostly in a straight band of stars across the center that encloses the core, as opposed to other spirals that have arms that twist all the way to their core. The Chandra data reveals compact objects like neutron stars or black holes pulling material from companion stars as well as the remnants of exploded stars. Additional data from Hubble (optical light) helps fill out the spiral arms with dust and gas, while Webb data shows dust and gas in the galaxy’s spiral arms. (X-ray: purple; optical: red, green, blue; infrared: red, green, blue)
The file is available at 147.40 millions of pixels for download at a resolution of 14400x10236 pixels.
Credits for X-ray: Chandra: NASA/CXC/SAO, XMM: ESA/XMM-Newton; for Infrared: JWST: NASA/ESA/CSA/STScI, Spitzer: NASA/JPL/CalTech; for Optical: Hubble: NASA/ESA/STScI, ESO; for Image Processing: L. Frattare, J. Major, and K. Arcand. Reconstruction and magnification via AI by PipploIMP.
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NGC 1672 - JWST - Chandra - Hubble - Magnification and reconstruction via AI.
Reconstruction using our artificial intelligence model from an image provided by Chandra X-ray Observatory about NGC 1672.
NGC 1672 is a spiral galaxy, but one that astronomers categorize as a “barred” spiral. In regions close to their centers, the arms of barred spiral galaxies are mostly in a straight band of stars across the center that encloses the core, as opposed to other spirals that have arms that twist all the way to their core. The Chandra data reveals compact objects like neutron stars or black holes pulling material from companion stars as well as the remnants of exploded stars. Additional data from Hubble (optical light) helps fill out the spiral arms with dust and gas, while Webb data shows dust and gas in the galaxy’s spiral arms. (X-ray: purple; optical: red, green, blue; infrared: red, green, blue)
The file is available at 147.40 millions of pixels for download at a resolution of 14400x10236 pixels.
Credits for X-ray: Chandra: NASA/CXC/SAO, XMM: ESA/XMM-Newton; for Infrared: JWST: NASA/ESA/CSA/STScI, Spitzer: NASA/JPL/CalTech; for Optical: Hubble: NASA/ESA/STScI, ESO; for Image Processing: L. Frattare, J. Major, and K. Arcand. Reconstruction and magnification via AI by PipploIMP.
Our Facebook Page: bit.ly/PipploFB
Our YouTube Channel: bit.ly/PipploYT