An independent determination of the local Hubble constant

被引:70
作者
Fernandez Arenas, David [1 ]
Terlevich, Elena [1 ]
Terlevich, Roberto [1 ,2 ]
Melnick, Jorge [3 ,4 ]
Chavez, Ricardo [5 ,6 ]
Bresolin, Fabio [7 ]
Telles, Eduardo [4 ]
Plionis, Manolis [8 ,9 ]
Basilakos, Spyros [10 ]
机构
[1] Inst Nacl Astrofis Opt & Electr, Puebla, Mexico
[2] Univ Cambridge, Inst Astron, Cambridge CB3 0HA, England
[3] European Southern Observ, Av Alonso de Cordova 3107, Santiago, Chile
[4] Observ Nacl, Rua Jose Cristino 77, BR-20921400 Rio De Janeiro, Brazil
[5] Univ Cambridge, Cavendish Lab, 19 JJ Thomson Ave, Cambridge CB3 0HE, England
[6] Univ Cambridge, Kavli Inst Cosmol, Madingley Rd, Cambridge CB3 0HA, England
[7] Univ Hawaii, Inst Astron, 2680 Woodlawn Dr, Honolulu, HI 96822 USA
[8] Natl Observ Athens P Pendeli, Athens, Greece
[9] Aristotle Univ Thessaloniki, Phys Dept, Thessaloniki 54124, Greece
[10] Acad Athens, Res Ctr Astron & Appl Math, Soranou Efessiou 4, Athens 11527, Greece
关键词
H II regions; galaxies: star formation; distance scale; cosmology: observations; H-II REGIONS; SPACE-TELESCOPE OBSERVATIONS; EQUATION-OF-STATE; CEPHEID DISTANCE; VELOCITY DISPERSIONS; PRECISION COSMOLOGY; GALACTIC CEPHEIDS; EMISSION-LINE; HII GALAXIES; KEY PROJECT;
D O I
10.1093/mnras/stx2710
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The relationship between the integrated H beta line luminosity and the velocity dispersion of the ionized gas of H II galaxies and giant H II regions represents an exciting standard candle that presently can be used up to redshifts z similar to 4. Locally it is used to obtain precise measurements of the Hubble constant by combining the slope of the relation obtained from nearby (z <= 0.2) H II galaxies with the zero-point determined from giant H II regions belonging to an 'anchor sample' of galaxies for which accurate redshift-independent distance moduli are available. We present new data for 36 giant H II regions in 13 galaxies of the anchor sample that includes the megamaser galaxy NGC 4258. Our data are the result of the first 4 yr of observation of our primary sample of 130 giant H II regions in 73 galaxies with Cepheid determined distances. Our best estimate of the Hubble parameter is 71.0 +/- 2.8(random) +/- 2.1(systematic) kms(-1) Mpc(-1). This result is the product of an independent approach and, although at present less precise than the latest SNIa results, it is amenable to substantial improvement.
引用
收藏
页码:1250 / 1276
页数:27
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