scholarly journals Anchors for the cosmic distance scale: the Cepheids U Sagittarii, CF Cassiopeiae, and CEab Cassiopeiae

2013 ◽  
Vol 560 ◽  
pp. A22 ◽  
Author(s):  
D. Majaess ◽  
G. Carraro ◽  
C. Moni Bidin ◽  
C. Bonatto ◽  
L. Berdnikov ◽  
...  
Nature ◽  
1958 ◽  
Vol 182 (4643) ◽  
pp. 1132-1133

1995 ◽  
Vol 10 ◽  
pp. 501-503
Author(s):  
George H. Jacoby

AbstractPlanetary nebula luminosity functions provide very accurate distances to galaxies as judged by comparisons with other techniques, including Cepheids; systematic effects cannot be significant. The method is empirical and is a consequence of the shallow initial-final mass relationship predicted by stellar evolution and directly measured. From distances to ∼ 30 galaxies, the PNLF yields H0 = 79, in excellent agreement with recent Cepheid discoveries in Virgo.


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