Journey to Star-forming Region Gum 19 in Vela | New Technology Telescope
The furnace that fuels Gum 19’s luminosity is a gigantic, superhot star called V391 Velorum. Shining brightest in the scorching blue range of visible light—V391 Velorum boasts a surface temperature in the vicinity of 30,000 degrees Celsius. Within the neighborhood of this fitful supergiant, new stars nonetheless continue to grow. In several million years—a blink of an eye in cosmic time—they will eventually reach the high density at their centers necessary to ignite nuclear fusion. The fresh outpouring of energy and stellar winds from these newborn stars will also modify the gaseous landscape of Gum 19.
The image is based on data obtained in three near-infrared bands (J, H, K; associated respectively to blue, green, and red). The image is 4.7 arcminutes across.
Release Date: March 31, 2010
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