(Annesastronomynews.com / Cienctec) the Herbig Haro object HH 47 is a bipolar stellar jet, with 4.

(Annesastronomynews.com / Cienctec) the Herbig Haro object HH 47 is a bipolar stellar jet, with 4.83 trillion miles long and 10 times greater than the width of the Solar System, and is located on the edge of the Gum Nebula, the approximately 1140 years-years minilink ericsson away from Earth in the constellation Vela. The Herbig-Haro minilink ericsson (HH) objects, which were named in honor of George Herbig and Guillermo astronomers minilink ericsson Haro are narrow jets of gas and matter that are ejected by young stars at speeds from 100 to 1000 kilometers per second and colliding minilink ericsson with clouds gas and dust nearby. They are a great region for the formation of stars, and some of them are seen around a single star, aligned along its axis of rotation. minilink ericsson Stellar jets seem to form as the cloud of dust and gas begins to make the movement of stars swirl and new escape. These objects are transient phenomena, lasting no more than a few thousand years. They can obviously develop into a short time scale, while moving rapidly away from its parent star, the gas clouds of interstellar space. The central low-mass protostar HH 47, which contains ice water and carbon dioxide, as well as organic molecules that are ejecting jet stream and creating a bipolar, in addition to locate within a Bok globule, or a nebula Dark containing very young stars. This image clearly reveals the extremely complicated pattern of the jet which indicates that the star (hidden within the dust cloud near the eastern edge of the image) can be stirred, stirring this possibly generated by the gravitational pull of a companion star. The jet has dug a hole through the dense cloud of gas and now travels at a high speed through interstellar space. Shock waves form when the jet collides with the interstellar gas, causing the jet to shine. The white filaments in the lower left reflect light of a newborn and obscured star. This image was taken with the Wide Field Planetary Camera 2 aboard the Hubble Space Telescope, and was created from data recorded in 1994, 1999 and 2008.
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