Hostname: page-component-6bf8c574d5-pdxrj Total loading time: 0 Render date: 2025-03-07T22:55:39.329Z Has data issue: false hasContentIssue false
  • English
  • Français

Surface Photometry of Galaxies in the Pisces-Perseus Region

Published online by Cambridge University Press:  26 July 2016

M. Watanabe ,
T. Ichikawa ,
M. Fukugita ,
K. Tarusawa  and
S. Okamura
M. Watanabe
Affiliation:
Department of Astronomy, School of Science†, University of Tokyo, Tokyo 113, Japan
T. Ichikawa
Affiliation:
Kiso Observatory, Institute of Astronomy, Faculty of Science, University of Tokyo, Nagano 397-01, Japan
M. Fukugita
Affiliation:
Yukawa Institute for Theoretical Physics, Kyoto University, Kyoto 606, Japan
K. Tarusawa
Affiliation:
Kiso Observatory, Institute of Astronomy, Faculty of Science, University of Tokyo, Nagano 397-01, Japan
S. Okamura
Affiliation:
Department of Astronomy, School of Science†, University of Tokyo, Tokyo 113, Japan

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We have obtained B-band photographic surface photometry of ∼ 2000 galaxies in the Pisces-Perseus region. Combining these photometry data with redshift and HI 21 cm line-width data for spiral galaxies in the region, we have studied the Hubble constant and large-scale peculiar motions. Taking biases into account quantitatively we obtain H0 = 80 ±9+17−22 km/s−1Mpc−1. The prevalent infalling motion in the region is found to be still controversial if the biases are carefully considered.

Type
Part Thirteen: Properties and Clustering of Galaxies and Clusters
Information
Symposium - International Astronomical Union , Volume 161: Astronomy from Wide-Field Imaging , 1994 , pp. 603 - 609
Copyright
Copyright © Kluwer 1994 

References

Bothun, G.D. et al., 1985. Astrophys. J. Suppl., 57, 423.Google Scholar
Burstein, D. et al., 1987. Astrophys. J. Suppl., 64, 601.Google Scholar
de Vaucouleurs, G. et al., 1991. ‘Third Reference Catalogue of Bright Galaxies (RC3)’ Springer-Verlag.Google Scholar
Dressler, A. et al., 1987. Astrophys. J. Lett., 313, L37.Google Scholar
Fukugita, M. et al., 1991. Astrophys. J., 376, 8.Google Scholar
Giovanelli, R. and Haynes, M.P., 1985. Astron. J., 90, 2445.Google Scholar
Giovanelli, R. and Haynes, M.P., 1989. Astron. J., 97, 633.CrossRefGoogle Scholar
Giovanelli, R. et al., 1986. Astron. J., 92, 250.CrossRefGoogle Scholar
Ichikawa, T. and Fukugita, M., 1992. Astrophys. J., 394, 61.Google Scholar
Ichikawa, T. and Watanabe, M., 1993. In preparation.Google Scholar
Longo, G. and de Vaucouleurs, A., 1983. ‘A General Catalogue of Photoelectric Magnitudes and Colors in the U, B, V System of 3,578 Galaxies Brighter than the 16th V-Magnitude (1936–1982)’, The University of Texas Monographs in Astronomy, No. 3.Google Scholar
Lynden-Bell, D. et al., 1988. Astrophys. J., 326, 19.Google Scholar
Nilson, P., 1973. ‘Uppsala General Catalogue of Galaxies (UGC)’, Acta Uppsala Univ. Ser. V:A, Vol 1.Google Scholar
Willick, J.A., 1990. Astrophys. J. Lett., 351, L5.CrossRefGoogle Scholar
Zwicky, F. et al., 1961–1968. ‘Catalogue of Galaxies and of Clusters of Galaxies (CGCG)’, L. Speich, Zurich.Google Scholar