Mostrando entradas con la etiqueta the Small Magellanic Cloud. Mostrar todas las entradas
Mostrando entradas con la etiqueta the Small Magellanic Cloud. Mostrar todas las entradas

domingo, 13 de noviembre de 2016

NASA : Hubble Takes Flight with the Toucan and the Cluster .- Telescopio Espacial Hubble toma vuelo con el Cluster del Tucán.....

http://www.nasa.gov/image-feature/goddard/2016/hubble-takes-flight-with-the-toucan-and-the-cluster
     
bright cluster of stars on a dark starfield
It may be famous for hosting spectacular sights such as the Tucana Dwarf Galaxy and 47 Tucanae (heic1510), the second brightest globular cluster in the night sky, but the southern constellation of Tucana (The Toucan) also possesses a variety of unsung cosmic beauties.

One such beauty is NGC 299, an open star cluster located within the Small Magellanic Cloud just under 200,000 light-years away. Open clusters such as this are collections of stars weakly bound by the shackles of gravity, all of which formed from the same massive molecular cloud of gas and dust. Because of this, all the stars have the same age and composition, but vary in their mass because they formed at different positions within the cloud.

This unique property not only ensures a spectacular sight when viewed through a sophisticated instrument attached to a telescope such as Hubble’s Advanced Camera for Surveys, but gives astronomers a cosmic laboratory in which to study the formation and evolution of stars — a process that is thought to depend strongly on a star’s mass.
Image credit: ESA/Hubble & NASA
Text credit: European Space Agency


Last Updated: Nov. 4, 2016
Editor: Karl Hille
NASA
Guillermo Gonzalo Sánchez Achutegui
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viernes, 8 de noviembre de 2013

NASA : Supernova SNR B0049-73.6


Supernova SNR B0049-73.6
The details of how massive stars explode remains one of the biggest questions in astrophysics. Located in the neighboring galaxy of the Small Magellanic Cloud, this supernova, SNR B0049-73.6, provides astronomers with another excellent example of such an explosion to study. Chandra observations of the dynamics and composition of the debris from the explosion support the view that the explosion was produced by the collapse of the central core of a star. In this image, X-rays from Chandra (purple) are combined with infrared data from the 2MASS survey (red, green, and blue).
Image credit: X-ray: NASA/CXC/Drew Univ/S.Hendrick et al, Infrared: 2MASS/UMass/IPAC-Caltech/NASA/NSF
NASA
Guillermo Gonzalo Sánchez Achutegui
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