Archivo de imágenes de Hubble
Imagen de brújula y escala para 30 Doradus IR
CreditsIllustration: NASA, ESA, and Z. Levay (STScI)
- Fecha
- Jan 1, 2014
- Misión
- Hubble Space Telescope
- ID de archivo
- hubblesite-images-2014-02-3285-image
Credits
Illustration: NASA, ESA, and Z. Levay (STScI)Detalles de la imagen
| About The Object | |
|---|---|
| Object Name | 30 Doradus |
| Object Description | Emission Nebula in the Large Magellanic Cloud |
| R.A. Position | 05h 38m 42.4s |
| Dec. Position | -69° 6' 3.35" |
| Constellation | Dorado |
| Distance | Approximately 170,000 light-years (52,000 parsecs) |
| About The Data | |
| Data Description | The ACS/WFC3 data are from the following HST proposals: : D. Lennon (ESA), E. Sabbi (ESA/STScI), J. Anderson, R. van der Marel, T. Sohn, and N. Walborn (STScI), L. Bedin (INAF, Padua), C. Evans (Royal Observatory Edinburgh), H. Sana (STScI/ESA), N. Langer (University of Bonn), S. de Mink (Carnegie Institution of Washington), P. Crowther (University of Sheffield), A. Herrero (IAC, Tenerife), N. Bastian (USM, Munich), and E. Bressert (Australia Telescope National Facility); : E. Sabbi (ESA/STScI), A. Aloisi, J. Anderson, K. Gordon, A. Koekemoer, R. van der Marel, N. Panagia, and C. Christian (STScI), M. Boyer (NASA/GSFC), C. Evans (Royal Observatory Edinburgh), J. Gallagher (University of Wisconsin, Madison), E. Grebel (Astronomisches Rechen-Institut Heidelberg), S. de Mink (Carnegie Institution of Washington), S. Larsen (Radboud Universiteit Nijmegen), D. Lennon (ESA), M. Tosi (INAF, Osservatorio Astronomico di Bologna), and D. Zaritsky (University of Arizona) |
| Instrument | HST>ACS/WFC, HST>WFC3/IR, and HST>WFC3/UVIS |
| Exposure Dates | October 2011 - April 2013 |
| Filters | ACS/WFC: F775W (i) WFC3/UVIS: F775W (i) WFC3/IR: F110W (J), F160W (H) |
| About The Image | |
| Color Info | The images in this release are composites of separate exposures obtained with the ACS and WFC3 instruments on the Hubble Space Telescope. Several filters were used to sample broad and narrow wavelength 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: Blue: F775W (i) Green: F110W (J) Red: F160W (H) |
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