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insula@macondo – leon

64dc615b-8093-4821-b922-3564ed1910fd

Posted in conciertos, Imagen format on 20/07/2018 by insula. Deja un comentario

insula@telefon_tel_aviv

http://giradiscos.org/post/171376885188/telefon-tel-aviv-ghostly-international-usa

Posted in Sin categoría on 30/03/2018 by insula. Deja un comentario

insula@fuachaval

https://es-es.facebook.com/events/190145651586057/

Posted in Sin categoría on 15/03/2018 by insula. Deja un comentario

INSULA@AMPOSTA

Posted in conciertos, videos, Imagen format on 25/07/2017 by insula. Deja un comentario

insula@toroide

Posted in Sin categoría, Imagen format on 21/06/2017 by insula. Deja un comentario

insula@espacio_vista

Posted in conciertos, Imagen format on 05/06/2017 by insula. Deja un comentario

insula@modularhaze

Posted in conciertos, Imagen format on 25/04/2017 by insula. Deja un comentario

insula@cargaydescarga
Posted in conciertos, videos on 25/04/2017 by insula. Deja un comentario

insula@zuloroom
Posted in videos on 14/03/2017 by insula. Deja un comentario

onoto@lucy_in_the_sky
This is a Hubble Space Telescope image (right) of a vast nebula called NGC 604, which lies in the neighboring spiral galaxy M33, located 2.7 million light-years away in the constellation Triangulum. This is a site where new stars are being born in a spiral arm of the galaxy. Though such nebulae are common in galaxies, this one is particularly large, nearly 1,500 light-years across. The nebula is so vast it is easily seen in ground-based telescopic images (left). At the heart of NGC 604 are over 200 hot stars, much more massive than our Sun (15 to 60 solar masses). They heat the gaseous walls of the nebula making the gas fluoresce. Their light also highlights the nebula's three-dimensional shape, like a lantern in a cavern. By studying the physical structure of a giant nebula, astronomers may determine how clusters of massive stars affect the evolution of the interstellar medium of the galaxy. The nebula also yields clues to its star formation history and will improve understanding of the starburst process when a galaxy undergoes a "firestorm" of star formation. The image was taken on January 17, 1995 with Hubble's Wide Field and Planetary Camera 2. Separate exposures were taken in different colors of light to study the physical properties of the hot gas (17,000 degrees Fahrenheit, 10,000 degrees Kelvin

facebook event

Posted in Sin categoría on 22/11/2016 by insula. Deja un comentario

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