About Galaxy Evolution Explorer Data Release

http://galex.stsci.edu/GR6/

Homepages about M 106

http://www.spacetelescope.org/news/heic1302/

http://www.spacetelescope.org/videos/heic1302c/

M 106 with giant black hole in his nucleus

Galex UV Images      Digital treatment Detthow G.G.

Image color table:
Image scaling:	Log, values range from 4.4326239731162786E-4  to 2.032351493835449
Image size(degrees):	0.249999996 x 0.249999996
Image size(pixels):	600 x 600
Requested Center:	m 106
Requested Center:	184.74008299999994, 47.303718999999994
Coordinate System:	J2000.0
Map projection:	Tan
Sampler:	NNSampler
Provenance:	All data is downloaded from  the MAST GALEX archive.
Copyright:	Public domain.

Digital image work  Detthow G.G. Software Salsa J and Sky view homepage.


3D Image

Isointensities

Image scaling:	Log, values range from 71.98657989501953 to 1764.0492858886719
Image size(degrees):	0.16666662000000002 x 0.16666662000000002
Image size(pixels):	600 x 600
Requested Center:	m 106
Requested Center:	184.74008299999994, 47.303718999999994
Coordinate System:	J2000.0
Map projection:	Tan
Sampler:	NNSampler
Provenance:	The Two Micron All Sky Survey is a joint project  of the University  of Massachusetts and the  Infrared Processing and Analysis Center, funded by the National Aeronautics  and Space Administration and the National Science Foundation.
Copyright:	Researchers are asked to include the following  acknowledgment in any  published material that makes use of data products from the Two Micron  All Sky Survey (2MASS):   "This publication makes use of data products from  the Two Micron All Sky Survey,  which is a joint project of the  University of Massachusetts  and the Infrared Processing and Analysis Center,  funded by the National Aeronautics and  Space  Administration and the National  Science Foundation."

Sky view

Image color table:
Image scaling:	Log, values range from 71.98657989501953 to 1764.0492858886719
Image size(degrees):	0.16666662000000002 x 0.16666662000000002
Image size(pixels):	600 x 600
Requested Center:	m 106
Requested Center:	184.74008299999994, 47.303718999999994
Coordinate System:	J2000.0
Map projection:	Tan
Sampler:	NNSampler
Provenance:	The Two Micron All Sky Survey is a joint project of the University  of Massachusetts and the Infrared Processing and Analysis Center,  funded by the National Aeronautics and Space Administration and the  National Science Foundation.
Copyright:	Researchers are asked to include the following acknowledgment in any  published material that makes use of data products the Two Micron All Sky Survey (2MASS):   "This publication makes use of data products from  the Two Micron All Sky Survey, which is a joint project of the  University of Massachusetts and the Infrared Processing and  Analysis Center, funded by the National  Aeronautics and Space Administration and the  National Science Foundation."

More information

M106 from the Hubble. Copyright: NASA, ESA, the Hubble Heritage Team (STScI/AURA),
 and R. Gendler (for the Hubble Heritage Team). Acknowledgment: J. GaBany,
A. van der Hoeven

Old Image, with new digital treatment

**********************NGC 5139**********************

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Júpiter from Botucatu

 

******************************Botucatu S.P.************************

 

 

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Kappa Crucis NGC 4755

Santos Dumont crater in Moon

                                         Copýright   http://www.santos-dumont.net/lua.htm

Santos-Dumont (crater)

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Santos-Dumont (crater)

Coordinates	27°42′N 4°48′E / 27.7°N 4.8°E / 27.7; 4.8Coordinates: 27°42′N 4°48′E / 27.7°N 4.8°E / 27.7; 4.8
Diameter	8 km
Depth	Unknown
Colongitude	356° at sunrise
Eponym	Alberto Santos-Dumont

Santos-Dumont is a small lunar impact crater that lies in the northern end of the Montes Apenninus range at the eastern edge of the Mare Imbrium. This feature was previously designated Hadley B prior to being given a name by the IAU. It is located about 30 kilometers to the northeast of Mons Hadley, a mountain massif.
This crater is a circular, bowl-shaped formation that is situated atop a ridge in the Montes Apenninus. It is otherwise an unremarkable formation with no unusual features and little appearance of wear.
To the northwest of Santos-Dumont is a 90-km-wide system of rilles designated the Rimae Fresnel, being named for the Promontorium Fresnel that lies to the north of the crater. This last formation forms the northern end of the Montes Apenninus, and lies astride the gap that joins the Mare Imbrium to the west with the Mare Serenitatis to the east. To the southeast, in the valley past Mons Hadley, is the landing site of the Apollo 15 mission.
This feature is named in honour of the Brazilian aviation pioneer Alberto Santos-Dumont.