scholarly journals 1.65  $\rm \mu$m(H-band) surface photometry of disk galaxies. I. Observations of 158 galaxies with the Calar Alto 2.2 m telescope

1996 ◽  
Vol 120 (3) ◽  
pp. 489-520 ◽  
Author(s):  
G. Gavazzi ◽  
D. Pierini ◽  
A. Boselli ◽  
R. Tuffs
Keyword(s):  
Disk Galaxies ◽  
Surface Photometry ◽  
Calar Alto

Optical Surface Photometry of a Sample of Disk Galaxies. I. Observations and Data Reduction

2000 ◽  
Vol 119 (4) ◽  
pp. 1638-1644 ◽  
Author(s):  
J. A. L. Aguerri ◽  
A. M. Varela ◽  
M. Prieto ◽  
C. Muñoz-Tuñón
Keyword(s):  
Data Reduction ◽  
Disk Galaxies ◽  
Surface Photometry ◽  
Optical Surface

Ultra-Deep Near Infrared Surface Photometry of Edge-on Disk Galaxies

2001 ◽  
pp. 329-329
Author(s):  
A. Guijarro ◽  
R. Peletier ◽  
R. De Grijs ◽  
J. Jiménez-Vicente ◽  
E. Battaner
Keyword(s):  
Near Infrared ◽  
Disk Galaxies ◽  
Surface Photometry

Structure and Morphology of Disk Galaxies with Visible and NIR Surface Photometry

2001 ◽  
pp. 129-132
Author(s):  
A. Guijarro ◽  
R. Peletier ◽  
R. De Grijs ◽  
J. Jiménez-Vicente ◽  
E. Battaner
Keyword(s):  
Disk Galaxies ◽  
Surface Photometry ◽  
Structure And Morphology

scholarly journals Optical surface photometry of a sample of disk galaxies

2001 ◽  
Vol 367 (2) ◽  
pp. 405-427 ◽  
Author(s):  
M. Prieto ◽  
J. A. L. Aguerri ◽  
A. M. Varela ◽  
C. Muñoz-Tuñón
Keyword(s):  
Disk Galaxies ◽  
Surface Photometry ◽  
Optical Surface

scholarly journals Surface Photometry of Pure Disk Galaxies

1984 ◽  
Vol 78 ◽  
pp. 385-387
Author(s):  
C. Carignan
Keyword(s):  
Star Formation ◽  
Disk Galaxies ◽  
Surface Photometry

AbstractSurface photometry from U.K.S.T.U. plates in U, BJ and RF is presented for the three Sculptor Group galaxies NGC 7793, NGC 247 and NGC 300. Their photometric parameters are derived and compared to those of M33. Our color maps are used to sort out the data into blue and red pixels where the blue pixels profiles are expected to be rather irregular, representative of the clumpy locations of areas of recent star formation while the red pixels profiles should approximate the smoother distribution of the old disk population.

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