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Contains:  Flaming Star nebula, IC 405
Getting plate-solving status, please wait...
AE Aurigae nebula - IC 405 [DSS-WISE], 





    
        

            Giuseppe Donatiello
AE Aurigae nebula - IC 405 [DSS-WISE]

AE Aurigae nebula - IC 405 [DSS-WISE]

Technical card

Resolution: 4439x5208

Dates:Jan. 25, 2015

Integration: 0.0 hours

Avg. Moon age: 5.58 days

Avg. Moon phase: 31.33%

Astrometry.net job: 515352

RA center: 78.919 degrees

DEC center: 34.145 degrees

Pixel scale: 1.008 arcsec/pixel

Orientation: 0.180 degrees

Field radius: 0.958 degrees

Description

Image credit: DSS - POSS-II(*) / IRSA - WISE(**) - NASA / JPL - Caltech / UCLA / Giuseppe Donatiello

Acknowledgments:
This image has made use of the NASA/ IPAC Infrared Science Archive, which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.
The Digitized Sky Survey (DSS) was produced at the Space Telescope Science Institute under U.S. Government grant NAG W-2166. The images of these surveys are based on photographic data obtained using the Oschin Schmidt Telescope on Palomar Mountain and the UK Schmidt Telescope. The plates were processed into the present compressed digital form with the permission of these institutions
(*) The Second Palomar Observatory Sky Survey (POSS-II) was made by the California Institute of Technology with funds from the National Science Foundation, the National Geographic Society, the Sloan Foundation, the Samuel Oschin Foundation, and the Eastman Kodak Corporation.
(**) This image makes use of data products from the Wide-field Infrared Survey Explorer (WISE), which is a joint project of the University of California, Los Angeles, and the Jet Propulsion Laboratory/California Institute of Technology, funded by the National Aeronautics and Space Administration.

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Giuseppe_Donatiello
Giuseppe Donatiello
License: None (All rights reserved)
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AE Aurigae nebula - IC 405 [DSS-WISE], 





    
        

            Giuseppe Donatiello