THE CEPHEID DISTANCE TO IC-4182 - CALIBRATION OF MV(MAX) FOR SN IA 1937C AND THE VALUE OF H0

被引:80
作者
SANDAGE, A
SAHA, A
TAMMANN, GA
PANAGIA, N
MACCHETTO, D
机构
[1] UNIV BASEL,INST ASTRON,CH-4102 BINNINGEN,SWITZERLAND
[2] EUROPEAN SO OBSERV,W-8046 GARCHING,GERMANY
[3] UNIV CATANIA,I-95125 CATANIA,ITALY
[4] SPACE TELESCOPE SCI INST,BALTIMORE,MD 21218
关键词
CEPHEIDS; DISTANCE SCALE; GALAXIES; INDIVIDUAL; IC-4182; SUPERNOVAE; 1937C;
D O I
10.1086/186657
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Cepheid variables with periods from 2 to more than 50 days have been found in IC 4182 from observations with the Hubble Space Telescope over a time interval of 47 days, comprised of 20 epochs. The period-luminosity relation from photometry of 27 Cepheids in the F555W HST magnitude system gives an apparent V distance modulus of (m - M)AV = 28.47 +/- 0.08. The absolute magnitude of the type Ia supernova 1937C is M(V)(max) = - 19.92 +/- 0.13 from these data. Combining this with the Hubble diagram for SN la gives a Hubble constant of H0 = 45 +/- 9 km s-1 Mpc-1. The inverse Hubble time is 22 Gyr. If q0 = 1/2, the age of the universe would be 15 GHr, with a formal uncertainty of +/-20%.
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页码:L7 / &
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