Archivo de imágenes de Hubble
Imagen de brújula y escala del Abell 520
CreditsIllustration: NASA, ESA, and Z. Levay (STScI); Image: NASA, ESA, CFHT, CXO, M.J. Jee (University of California, Davis), and A. Mahdavi (San Francisco State University)
- Fecha
- Jan 1, 2012
- Misión
- Hubble Space Telescope
- ID de archivo
- hubblesite-images-2012-10-2985-image
Credits
Illustration: NASA, ESA, and Z. Levay (STScI);Image: NASA, ESA, CFHT, CXO, M.J. Jee (University of California, Davis), and A. Mahdavi (San Francisco State University)
Detalles de la imagen
| About The Object | |
|---|---|
| Object Name | Abell 520 |
| Object Description | Merging Galaxy Cluster |
| R.A. Position | 04h 54m 18.98s |
| Dec. Position | 02° 56' 48.8" |
| Constellation | Orion |
| Distance | 2.4 billion light-years (740 million parsecs) |
| About The Data | |
| Data Description | The image was created from Hubble data from proposal : J. Dalcanton (University of Washington, Seattle), A. Mahdavi (San Francisco State University), H. Hoekstra (Leiden Observatory), and A. Babul (University of Victoria, BC). The science paper is led by M.J. Jee (University of California, Davis). |
| Instrument | HST>WFPC2, CFHT, and Chandra |
| Exposure Dates | August 19-22, 2008, Exposure Time: 11 hours |
| Filters | CFHT (B), CFHT (V), HST/WFPC2 F814W (I), and CXO X-ray |
| About The Image | |
| Color Info | This image is a composite of separate exposures acquired by the HST/WFPC2 instrument, the Canada-France-Hawaii Telescope (CFHT), and the Chandra X-ray Observatory. Several filters were used to sample various wavelength and energy ranges. The color results from assigning different hues (colors) to each monochromatic (grayscale) image associated with an individual filter. In this case, the assigned colors are: White (visible): CFHT (B) + CFHT (V) + HST/WFPC2 F814W (I) Red (luminosity): CFHT Blue: HST/WFPC2 F814W (I) Green: CXO X-ray |
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Fuente
La imagen y el material de referencia se acreditan al archivo oficial de la misión enlazado a continuación.
Ver en NASA.gov
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