1999ApJ...515...29M


Query : 1999ApJ...515...29M

1999ApJ...515...29M - Astrophys. J., 515, 29-41 (1999/April-2)

The Hubble space telescope key project on the extragalactic distance scale. XV. A cepheid distance to the Fornax cluster and its implications.

MADORE B.F., FREEDMAN W.L., SILBERMANN N., HARDING P., HUCHRA J., MOULD J.R., GRAHAM J.A., FERRARESE L., GIBSON B.K., HAN M., HOESSEL J.G., HUGHES S.M., ILLINGWORTH G.D., PHELPS R., SAKAI S. and STETSON P.

Abstract (from CDS):

Using the Hubble Space Telescope, 37 long-period Cepheid variables have been discovered in the Fornax Cluster spiral galaxy NGC 1365. The resulting V and I period-luminosity relations yield a true distance modulus of µ0=31.35±0.07 mag, which corresponds to a distance of 18.6±0.6 Mpc. This measurement provides several routes for estimating the Hubble constant. (1) Assuming this distance for the Fornax Cluster as a whole yields a local Hubble constant of 70±18 (random) ±7 (systematic) km.s–1.Mpc–1. (2) Nine Cepheid-based distances to groups of galaxies out to and including the Fornax and Virgo Clusters yield H0=73±16 (random) ±7 (systematic) km.s–1.Mpc–1. (3) Recalibrating the I-band Tully-Fisher relation using NGC 1365 and six nearby spiral galaxies, and applying it to 15 galaxy clusters out to 100 Mpc, give H0=76±3 (random) ±8 (systematic) km.s–1.Mpc–1. (4) Using a broad-based set of differential cluster distance moduli ranging from Fornax to Abell 2147 gives H0=72±3 (random) ±6 (systematic) km.s–1.Mpc–1. Finally, (5) assuming the NGC 1365 distance for the two additional Type Ia supernovae in Fornax and adding them to the SN Ia calibration (correcting for light-curve shape) gives H0=67±6 (random) ±7 (systematic) km.s–1.Mpc–1 out to a distance in excess of 500 Mpc. All five of these H0 determinations agree to within their statistical errors. The resulting estimate of the Hubble constant, combining all of these determinations, is H0=72±5 (random) ±7 (systematic) km.s–1.Mpc–1. An extensive tabulation of identified systematic and statistical errors, and their propagation, is given.

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Journal keyword(s): Stars: Variables: Cepheids - Cosmology: Distance Scale - Galaxies: Clusters: Individual: Name: Fornax - Galaxies: Distances and Redshifts - Galaxies: Individual: NGC Number: NGC 1365

Simbad objects: 43

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Number of rows : 43
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 M 31 AGN 00 42 44.330 +41 16 07.50 4.86 4.36 3.44     ~ 13622 1
2 NGC 300 GiG 00 54 53.4465638304 -37 41 03.168402396 8.83 8.69 8.13 7.46   ~ 1614 2
3 M 33 GiG 01 33 50.8965749232 +30 39 36.630403128 6.17 6.27 5.72     ~ 6226 1
4 NGC 925 H2G 02 27 16.913 +33 34 43.97   10.69 10.12 9.55   ~ 818 1
5 NAME NGC 1023 Group GrG 02 39 37.9 +39 20 51           ~ 81 0
6 NGC 1316 rG 03 22 41.789 -37 12 29.52 9.81 9.15 8.53 7.66   ~ 1491 1
7 SN 1980N SN* 03 23 00.319 -37 12 49.90   12.5 12.37     SNIa 159 1
8 NGC 1326A AG? 03 25 08.50 -36 21 50.2   13.80   12.91 13.7 ~ 103 0
9 NGC 1365 Sy1 03 33 36.458 -36 08 26.37 10.48 10.08 9.63 8.79 9.7 ~ 1987 2
10 SN 1992A SN* 03 36 27.41 -34 57 31.4   12.56 12.50     SNIa 409 1
11 NGC 1380 Sy2 03 36 27.590 -34 58 34.68 11.32 10.94 9.93 9.37   ~ 460 1
12 ACO S 373 ClG 03 38 29.4 -35 27 08           ~ 2029 0
13 NGC 1425 EmG 03 42 11.4831633240 -29 53 36.186684252   11.61   11.6 10.9 ~ 209 0
14 NGC 2090 GiG 05 47 01.8557074752 -34 15 01.679264784 12.17 11.70 11.20 10.43 11.0 ~ 206 1
15 NGC 2363A HII 07 28 42.8 +69 11 21           ~ 588 3
16 NGC 2366 H2G 07 28 52.4529 +69 12 38.859 12.25 11.86 11.39 11.33   ~ 801 0
17 NGC 2403 AGN 07 36 51.3381434280 +65 36 09.650825640 9.31 8.84 8.38 8.19   ~ 1887 1
18 NAME M 81-82 Group GrG 09 55 +69.1           ~ 758 0
19 M 81 Sy2 09 55 33.1726556496 +69 03 55.062505368   7.89 6.94     ~ 4725 3
20 NGC 3109 AG? 10 03 06.877 -26 09 34.46 11.10 10.42 10.04 9.91   ~ 825 2
21 NAME M 96 Group GrG 10 46 45 +11 49.1           ~ 330 0
22 NGC 3621 Sy2 11 18 16.300 -32 48 45.36 10.10 9.44 9.56 8.07 10.1 ~ 661 3
23 SN 1973R SN* 11 20 11.5 +12 59 55   15.3 11.8     SNIIP 80 1
24 SN 1989B SN* 11 20 13.93 +13 00 18.9   12.25       SNIa 372 1
25 M 66 AGN 11 20 15.0 +12 59 29 9.85 9.65 8.92     ~ 1509 4
26 M 109 GiG 11 57 35.9631479640 +53 22 29.006082336   10.94   9.57   ~ 483 0
27 M 100 AGN 12 22 54.9299993592 +15 49 20.296257960 10.04 10.05 9.35     ~ 1963 2
28 SN 1974G SN* 12 26 27.1 +31 13 24   12.48       SNIa 101 1
29 NGC 4414 GiC 12 26 27.1276893168 +31 13 24.626206488 11.12 10.96 10.12     ~ 593 2
30 NAME Virgo Cluster ClG 12 30 47.8 +12 23 07           ~ 7107 0
31 NGC 4496 GiP 12 31 39.2222392512 +03 56 21.641352828   11.71       ~ 376 0
32 SN 1960F SN* 12 31 42.05 +03 56 47.7   11.34 11.43     SNIa 116 1
33 M 88 Sy2 12 31 59.1525062448 +14 25 13.148971824   14.33 13.18     ~ 843 1
34 NGC 4536 H2G 12 34 27.12887 +02 11 16.3680 11.14 11.16 10.55 17.393   ~ 913 3
35 SN 1981B SN* 12 34 29.57 +02 11 59.3   11.74       SNIa 416 1
36 NGC 4639 Sy1 12 42 52.3785000336 +13 15 26.706153600   13.62 12.72     ~ 642 0
37 SN 1990N SN* 12 42 56.68 +13 15 23.4   12.69 12.62     SNIa 406 1
38 IC 4182 BiC 13 05 48.7478324064 +37 36 12.965157684   11.86   11.40   ~ 344 1
39 SN 1937C SN* 13 05 53.2 +37 36 07   8.80 8.77     SNIa 203 1
40 SN 1972E SN* 13 39 52.7 -31 40 09   8.49 8.30     SNIa 309 1
41 NGC 5253 rG 13 39 55.990 -31 38 24.11 11.48 10.94 10.49 10.33 13.47 ~ 1421 4
42 M 101 GiP 14 03 12.583 +54 20 55.50   8.46 7.86 7.76   ~ 3138 2
43 NGC 7331 LIN 22 37 04.0506038088 +34 24 56.800076508 10.65 10.35 9.48     ~ 1284 2

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