A photometric and kinematic study of the barred spiral galaxy NGC 253. I - Detailed surface photometry

1980 ◽  
Vol 239 ◽  
pp. 54 ◽  
Author(s):  
W. D. Pence
Keyword(s):  
Spiral Galaxy ◽  
Surface Photometry ◽  
Kinematic Study ◽  
Detailed Surface ◽  
Barred Spiral Galaxy

scholarly journals Surface Photometry of Spiral Galaxy NGC 5005 and Elliptical Galaxy NGC 4278

2018 ◽  
Vol 15 (3) ◽  
pp. 314-323
Author(s):  
Baghdad Science Journal
Keyword(s):  
Spiral Galaxy ◽  
Surface Brightness ◽  
Elliptical Galaxy ◽  
Position Angle ◽  
Sloan Digital Sky Survey ◽  
Surface Photometry ◽  
Contour Maps ◽  
Sky Survey ◽  
Flat Field ◽  
The Galaxy

Two galaxies have been chosen, spiral galaxy NGC 5005 and elliptical galaxy NGC 4278 to study their photometric properties by using surface photometric techniques with griz-Filters. Observations are obtained from the Sloan Digital Sky Survey (SDSS). The data reduction of all images have done, like bias and flat field, by SDSS pipeline. The overall structure of the two galaxies (a bulge, a disk), together with isophotal contour maps, surface brightness profiles and a bulge/disk decomposition of the galaxy images were performed, although the disk position angle, ellipticity and inclination of the galaxies have been estimated.

scholarly journals Study of the Gas Kinematics in the Center of the Barred Spiral Galaxy NGC 4258.

1996 ◽  
Vol 157 ◽  
pp. 164-167
Author(s):  
S. N. Dodonov
Keyword(s):  
Spiral Galaxy ◽  
Spatial Sampling ◽  
Kinematic Structure ◽  
Gas Kinematics ◽  
Barred Spiral Galaxy ◽  
Integral Field Spectrograph ◽  
Integral Field

AbstractIntegral Field Spectrograph observations of southeast (SE) gas outflow in the center (11×13 arcsec) of NGC 4258 with spatial sampling 0.6 and 1.2 arcsec were made with the 6-m Telescope. Reconstructed spatial and kinematic structure of the SE outflow from 20-30 pc to 200-220 pc are presented.

Is NGC 4631 a barred spiral galaxy?

1991 ◽  
Vol 101 ◽  
pp. 825 ◽  
Author(s):  
Jean-Rene Roy ◽  
Jianguo Wang ◽  
Robin Arsenault
Keyword(s):  
Spiral Galaxy ◽  
Barred Spiral Galaxy

The velocity field of the barred spiral galaxy NGC 5383

1978 ◽  
Vol 219 ◽  
pp. 31 ◽  
Author(s):  
C. J. Peterson ◽  
N. Thonnard ◽  
V. C. Rubin ◽  
W. K., Jr. Ford
Keyword(s):  
Velocity Field ◽  
Spiral Galaxy ◽  
Barred Spiral Galaxy

Detailed study of the barred spiral galaxy NGC 4027. I - Photometry

1985 ◽  
Vol 298 ◽  
pp. 560 ◽  
Author(s):  
W. C. Pence ◽  
G. de Vaucouleurs
Keyword(s):  
Spiral Galaxy ◽  
Barred Spiral Galaxy

scholarly journals GMC evolution in a barred spiral galaxy with star formation and thermal feedback

2016 ◽  
Vol 461 (2) ◽  
pp. 1684-1700 ◽  
Author(s):  
Yusuke Fujimoto ◽  
Greg L. Bryan ◽  
Elizabeth J. Tasker ◽  
Asao Habe ◽  
Christine M. Simpson
Keyword(s):  
Star Formation ◽  
Spiral Galaxy ◽  
Thermal Feedback ◽  
Barred Spiral Galaxy

scholarly journals Hydrodynamical simulations of the barred spiral galaxy NGC 1097

2012 ◽  
Vol 10 (H16) ◽  
pp. 376-376
Author(s):  
Lien-Hsuan Lin ◽  
Hsiang-Hsu Wang ◽  
Pei-Ying Hsieh ◽  
Ronald E. Taam ◽  
Chao-Chin Yang ◽  
...  
Keyword(s):  
Spiral Galaxy ◽  
Gas Flow ◽  
Elliptical Galaxy ◽  
The Self ◽  
Two Dimensional ◽  
Nuclear Ring ◽  
Barred Spiral Galaxy ◽  
Circumnuclear Disk ◽  
Hydrodynamical Simulations ◽  
Self Gravity

AbstractNGC 1097 is a nearby barred spiral galaxy believed to be interacting with the elliptical galaxy NGC 1097A located to its northwest. It hosts a Seyfert 1 nucleus surrounded by a circumnuclear starburst ring. Two straight dust lanes connected to the ring extend almost continuously out to the bar. The other ends of the dust lanes attach to two main spiral arms. To provide a physical understanding of its structural and kinematical properties, two-dimensional hydrodynamical simulations have been carried out. Numerical calculations reveal that many features of the gas morphology and kinematics can be reproduced provided that the gas flow is governed by a gravitational potential associated with a slowly rotating strong bar. By including the self-gravity of the gas disk in our calculation, we have found the starburst ring to be gravitationally unstable which is consistent with the observation in Hsieh et al. (2011). Our simulations also show that gas can flow into the region within the starburst ring even after its formation, leading to the coexistence of both a nuclear ring and a circumnuclear disk.

Sign in / Sign up

Export Citation Format

Share Document