Archivo de imágenes de Hubble

Movimientos estelares de las estrellas Halo en la Vía Láctea

This illustration shows the disk of our Milky Way galaxy, surrounded by a faint, extended halo of old stars. Astronomers using the Hubble Space Telescope to observe the nearby Andromeda galaxy serendipitously identified a dozen foreground stars in the Milky Way halo. They measure...

Fecha
Jan 1, 2013
Misión
Hubble Space Telescope
ID de archivo
hubblesite-images-2013-07-3146-image
Por

This illustration shows the disk of our Milky Way galaxy, surrounded by a faint, extended halo of old stars. Astronomers using the Hubble Space Telescope to observe the nearby Andromeda galaxy serendipitously identified a dozen foreground stars in the Milky Way halo. They measured the first sideways motions (represented by the arrows) for such distant halo stars. The motions indicate the possible presence of a shell in the halo, which may have formed from the accretion of a dwarf galaxy. This observation supports the view that the Milky Way has undergone continuing growth and evolution over its lifetime by consuming smaller galaxies.

Credits

Illustration: NASA, ESA, and A. Feild (STScI);
Science: NASA, ESA, A. Deason and P. Guhathakurta (University of California, Santa Cruz), and R. van der Marel, T. Sohn, and T. Brown (STScI)

Detalles de la imagen

About The Object
Object NameMilky Way Halo
Object DescriptionMilky Way Shell Structure
About The Data
Data DescriptionThe Hubble data used in this science finding are from proposals and , PI: T. Brown (STScI), and , PI: R. van der Marel (STScI). The science team consists of: A. Deason and P. Guhathakurta (University of California, Santa Cruz), and R. van der Marel, T. Sohn, and T. Brown (STScI).
InstrumentHST>ACS/WFC and HST>WFC3/UVIS
Exposure DatesDecember 2002 - January 2003, August 2004 - January 2005, January - August 2010
FiltersF606W (V) and F814W (I)

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