Hubble constant at intermediate redshift using the CO-line Tully-Fisher relation

被引：11

作者：

Tutui, Y ^{[1
]}

Sofue, Y

Honma, M

Takashi, I

Wakamatsu, K

机构：

[1] Univ Tokyo, Inst Astron, Mitaka, Tokyo 1810015, Japan

[2] NHK Japan Broadcasting Corp, Program Prod Dept, Sci & Environm Div, Shibuya Ku, Tokyo 1508001, Japan

[3] Natl Astron Observ, VERA Project Off, Mitaka, Tokyo 1818588, Japan

[4] Tohoku Univ, Inst Astron, Aoba Ku, Sendai, Miyagi 9808578, Japan

[5] Gifu Univ, Dept Technol, Gifu 50111, Japan

来源：

PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN | 2001年 / 53卷 / 05期

基金：

日本学术振兴会;

关键词：

cosmology : Hubble constant; galaxies : distances and redshifts; ISM : CO line;

D O I：

10.1093/pasj/53.5.701

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We have determined distances and Hubble ratios for galaxies at intermediate redshifts, cz similar to 10000 to 35000 km s(-1), by applying the CO-line Tully-Fisher relation to our (CO)-C-12 (J = 1-0)-line observations using the Nobeyama 45-m telescope, and near-IR (NIR) photometry in the J- and H-bands using the 1.88-m telescope at Okayama Astrophysical Observatory. By averaging the Hubble ratios from the J-band result, we obtained a Hubble constant of H-0 = 60 +/- 10 kms(-1) Mpc(-1). We argue that the CO line-NIR Tully-Fisher relation can be a complimentary method to the other methods for measuring the distances of galaxies at intermediate and high redshifts.

引用

页码：701 / 712

页数：12

共 43 条

[41] Surface photometric calibration of the infrared Tully-Fisher relation using Cepheid-based distances of galaxies [J].