Archivo de imágenes de Hubble

Imagen del Hubble ACS de NGC 1275

This Hubble Space Telescope image of galaxy NGC 1275 reveals the fine, thread-like filamentary structures in the gas surrounding the galaxy. The red filaments are composed of cool gas being suspended by a magnetic field, and are surrounded by the 100-million-degree Fahrenheit hot...

Fecha
Jan 1, 2008
Misión
Hubble Space Telescope
ID de archivo
hubblesite-images-2008-28-2375-image
Por

This Hubble Space Telescope image of galaxy NGC 1275 reveals the fine, thread-like filamentary structures in the gas surrounding the galaxy. The red filaments are composed of cool gas being suspended by a magnetic field, and are surrounded by the 100-million-degree Fahrenheit hot gas in the center of the Perseus galaxy cluster.

The filaments are dramatic markers of the feedback process through which energy is transferred from the central massive black hole to the surrounding gas. The filaments originate when cool gas is transported from the center of the galaxy by radio bubbles that rise in the hot interstellar gas.

At a distance of 230 million light-years, NGC 1275 is one of the closest giant elliptical galaxies and lies at the center of the Perseus cluster of galaxies.

The galaxy was photographed in July and August 2006 with the Advanced Camera for Surveys in three color filters.

Credits

NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration;
Acknowledgment: A. Fabian (Institute of Astronomy, University of Cambridge, UK)

Detalles de la imagen

About The Object
Object NameNGC 1275, Perseus A, 3C 84
Object DescriptionActive Galaxy
R.A. Position03h 19m 48.15s
Dec. Position41° 30' 42.09"
ConstellationPerseus
DistanceAbout 230 million light-years (70 Megaparsecs)
DimensionsThe image is roughly 4 arcminutes (260,000 light-years or 78,000 parsecs) across.
About The Data
Data DescriptionHST Proposal: A. Fabian and C. Crawford (Institute of Astronomy, University of Cambridge, UK), C. Conselice (University of Nottingham), and J. Gallager and E. Zweibel (University of Wisconsin, Madison).
InstrumentHST>ACS/WFC
Exposure DatesJuly and August, 2006
FiltersF435W (B), F550W (V), and F625W (r)
About The Image
Color InfoThese images are a composite of separate exposures made by the ACS instrument on the Hubble Space Telescope. Three filters were used to sample various broad wavelength ranges. The color results from assigning different hues (colors) to each monochromatic image. In this case, the assigned colors are: Blue: F435W (B) Green: F550W (V) Red: F625W (r)

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