scholarly journals B and V CCD Photometry of Southern, Extreme Late-Type Spiral Galaxies

1997 ◽  
Vol 114 ◽  
pp. 1899 ◽  
Author(s):  
Lynn D. Matthews ◽  
John S., III Gallagher
2016 ◽  
Vol 464 (2) ◽  
pp. 1903-1922 ◽  
Author(s):  
Veselina Kalinova ◽  
Glenn van de Ven ◽  
Mariya Lyubenova ◽  
Jesús Falcón-Barroso ◽  
Dario Colombo ◽  
...  

2004 ◽  
Vol 127 (1) ◽  
pp. 105-118 ◽  
Author(s):  
Torsten Bker ◽  
Marc Sarzi ◽  
Dean E. McLaughlin ◽  
Roeland P. van der Marel ◽  
Hans-Walter Rix ◽  
...  

1999 ◽  
Vol 186 ◽  
pp. 491-491
Author(s):  
Xiaolei Zhang

The results from Hubble Space Telescope's Medium Deep Survey and Deep Fields indicate that there exists far more blue spiral galaxies at the intermediate and high redshifts than at the present epoch. A natural question therefore is: what have become of these excess late type galaxies as the Universe aged?


1988 ◽  
Vol 95 ◽  
pp. 408 ◽  
Author(s):  
C. Giovanardi ◽  
L. K. Hunt

1987 ◽  
Vol 63 ◽  
pp. 771 ◽  
Author(s):  
Isabella M. Gioia ◽  
Giuseppina Fabbiano

2006 ◽  
Vol 132 (4) ◽  
pp. 1426-1444 ◽  
Author(s):  
Kristine Spekkens ◽  
Riccardo Giovanelli
Keyword(s):  

1998 ◽  
Vol 116 (3) ◽  
pp. 1169-1185 ◽  
Author(s):  
L. D. Matthews ◽  
W. van Driel ◽  
J. S. Gallagher III

1983 ◽  
Vol 100 ◽  
pp. 69-76
Author(s):  
P. C. van der Kruit ◽  
G. S. Shostak

Most studies of the mass distribution in spiral galaxies have been based on the observed rotation curves. A serious ambiguity in this approach has always been that the rotation curve contains in itself no information on the mass distribution in the direction perpendicular to the galactic plane. The usual assumption has been that the mass in late type galaxies is distributed as the light, namely outside the central bulge in a highly flattened disk. In recent years it has been found that the rotation curves decline little or not at all, indicating large increases in the local value of M/L with increasing galactocentric radius (e.g. Bosma and van der Kruit, 1979). On the basis of dynamical arguments involving stability it has been suspected that the material giving rise to the large values of M/L - the “dark matter” - is distributed in the halos of these galaxies, so that the assumption of a flat mass distribution would have to be wrong.


2007 ◽  
Vol 466 (3) ◽  
pp. 905-916 ◽  
Author(s):  
K. Fathi ◽  
J. E. Beckman ◽  
A. Zurita ◽  
M. Relaño ◽  
J. H. Knapen ◽  
...  

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