Apr 3
LMC N44C, Within the Large Magellanic Cloud
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LMC N44C, Within the Large Magellanic Cloud
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Cloudscape in Large Magellanic Cloud ©
The Tarantula Nebula (30 Doradus, top) in the LMC // Cankun Wang
Thick clouds of cold hydrogen gas dominate this view of N159 from the Hubble Space Telescope, forming a complex network of ridges, cavities, and glowing filaments. Embedded within these dense clouds, newly formed stars shine, their intense light causing the surrounding hydrogen to glow in deep red tones.
The brightest regions mark the presence of hot, massive young stars whose powerful stellar winds and energetic light reshape their environment. These forces carve out bubble-like structures and hollowed cavities in the gas, and are clear signatures of stellar feedback in action. Dark clouds in the foreground are lit from behind by new stars.
N159 is one of the most massive star-forming clouds in the Large Magellanic Cloud, a dwarf galaxy that is the largest of the small galaxies that orbit our Milky Way. This image shows just a portion of this expansive star-forming complex, as the entire complex stretches over 150 light-years across.
Credit: ESA, NASA, R. Indebetouw.
Milky Way at York, Western Australia
Nikon d810a - 50mm - ISO 6400 - f/2.5 - Foreground: 7 x 30 seconds - Sky: 35 x 30 seconds - iOptron SkyTracker - Hoya Red Intensifier filter
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Large Magellanic Cloud
Henize 70: A SuperBubble In The LMC - June 13th, 1998.
"Stars with tens of times the mass of the Sun profoundly affect their galactic environment. Churning and mixing the interstellar gas and dust clouds, they leave their mark in the compositions and locations of future generations of stars and star systems. Dramatic evidence of this is beautifully illustrated in our neighboring galaxy, the Large Magellanic Cloud (LMC), by the lovely ring shaped nebula, Henize 70. It is actually a luminous "superbubble" of interstellar gas about 300 light-years in diameter, blown by winds from massive stars and supernova explosions, its interior filled with tenuous hot expanding gas. These superbubbles offer astronomers a chance to explore this crucial connection between the life cycles of stars and the evolution of galaxies."
© NASA
© NASA
© Dieter Willasch
© NASA
© Pea Mauro
© NASA
© Kavan Chay
honestly don't know why i'm posting this. i guess i have nothing else to do or to live for