Explanation: High-speed outflows of molecular gas from a pair of actively forming young stars shine in infrared light, revealing themselves in this NIRcam image from the James Webb Space Telescope. Cataloged as HH (Herbig-Haro) 46/47, the young stars are lodged within a dark nebula that is largely opaque when viewed in visible light. The pair lie at the center of the prominent reddish diffraction spikes in the NIRcam image. Their energetic stellar jets extend for nearly a light-year, burrowing into the dark interstellar material. A tantalizing object to explore with Webb's infrared capabilities, this young star system is relatively nearby, located only some 1,140 light-years distant in the nautical constellation Vela.

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Authors & editors: Robert Nemiroff (MTU) & Jerry Bonnell (USRA)
NASA Web Site Statements, Warnings, and Disclaimers
NASA Official: Jay Norris. Specific rights apply.
A service of: LHEA at NASA / GSFC
& Michigan Tech. U.

Publikacii s klyuchevymi slovami: Herbig-Haro object - Ob'ekt Herbiga-Aro Publikacii so slovami: Herbig-Haro object - Ob'ekt Herbiga-Aro
Sm. takzhe: HH 211: dzhety ot formiruyusheisya zvezdy HH 666: pylevoi stolb s dzhetom v Kile Dzhety v ob'ekte Herbiga-Aro 24 Dugi, dzhety i udarnye volny okolo NGC 1999 Molodye solnca v NGC 7129 Herbig-Aro 24 Puchok chastic formiruet HH 24 Vse publikacii na tu zhe temu >>