Candidate Galaxies for Study of the Local Velocity Field and Distance Scale Using Space Telescope - Part Two - the More Difficult Cases

1985 ◽  
Vol 90 ◽  
pp. 2001 ◽  
Author(s):  
A. Sandage ◽  
J. Bedke
1996 ◽  
Vol 168 ◽  
pp. 163-173 ◽  
Author(s):  
G. A. Tammann ◽  
Allan Sandage

The methods are reviewed that give a distance modulus to the core of the Virgo cluster of m - M = 31.64 ± 0.08 (D = 21.3 ± 0.8 Mpc). It is shown that the cosmic velocity of the cluster core is 1179 ± 17 km s−1, which, when combined with the distance gives Ho= 55 ± 3 km s−1Mpc−1from the Virgo cluster data alone. Nine independent methods are reviewed that confirm that Ho= 50 ± 2. Discussion is made why all methods that are said to give the short distance scale (Ho~ 85) are incorrect.


1999 ◽  
Vol 521 (1) ◽  
pp. 155-178 ◽  
Author(s):  
L. M. Macri ◽  
J. P. Huchra ◽  
P. B. Stetson ◽  
N. A. Silbermann ◽  
W. L. Freedman ◽  
...  

1994 ◽  
Vol 428 ◽  
pp. 143 ◽  
Author(s):  
Shaun M. G. Hughes ◽  
Peter B. Stetson ◽  
Anne Turner ◽  
Robert C., Jr. Kennicutt ◽  
Robert Hill ◽  
...  

1996 ◽  
Vol 463 ◽  
pp. 26 ◽  
Author(s):  
Daniel D. Kelson ◽  
Garth D. Illingworth ◽  
Wendy F. Freedman ◽  
John A. Graham ◽  
Robert Hill ◽  
...  

2008 ◽  
Author(s):  
Karen Masters ◽  
Robert Minchin ◽  
Emmanuel Momjian

Sign in / Sign up

Export Citation Format

Share Document