Surface photometry of disk galaxies at 60 and 100 microns - Radial gradients in dust temperature in optically thin disks

1992 ◽  
Vol 103 ◽  
pp. 1484 ◽  
Author(s):  
Gregory D. Bothun ◽  
C. Rogers
Keyword(s):  
Disk Galaxies ◽  
Surface Photometry ◽  
Dust Temperature ◽  
Thin Disks

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 Metal-rich infall onto the inner disk through the interaction between bulge winds and gaseous halos

2009 ◽  
Vol 5 (S265) ◽  
pp. 384-385
Author(s):  
Takuji Tsujimoto ◽  
Kenji Bekki
Keyword(s):  
Numerical Simulations ◽  
Chemical Evolution ◽  
Galactic Disk ◽  
Vital Role ◽  
Solar Neighborhood ◽  
Disk Galaxies ◽  
Chemical Abundances ◽  
Hydrodynamical Interaction ◽  
Thin Disks ◽  
First Time

AbstractWe demonstrate for the first time that gaseous halos of disk galaxies can play a vital role in recycling metal-rich gas ejected from the bulges and thus in promoting the chemical evolution of the disks. Our numerical simulations show that metal-rich bulge winds can be accreted onto the thin disks owing to hydrodynamical interaction between the gaseous ejecta and the gaseous halos. Accordingly, we anticipate that chemical abundances of the inner disk stars are significantly influenced by the enriched winds. About ~1% of gaseous ejecta from the bulges can be accreted onto the middle disk corresponding to the sun's position. We discuss these results in the context of the origin of super metal-rich stars in the solar neighborhood as well as an observed flattening of the abundance gradient in the Galactic disk.

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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