Near infrared surface photometry of late-type Virgo cluster galaxies

被引：70

作者：

Boselli, A

Tuffs, RJ

Gavazzi, G

Hippelein, H

Pierini, D

机构：

[1] MAX PLANCK INST KERNPHYS, D-69117 HEIDELBERG, GERMANY

[2] OBSERV PARIS, DEMIRM, F-75014 PARIS, FRANCE

[3] CNRS, ASTRON SPATIALE LAB, TRAVERSE SIPHON, F-13376 MARSEILLE 12, FRANCE

[4] UNIV MILAN, I-20133 MILAN, ITALY

[5] OSSERV ASTRON BRERA, I-20121 MILAN, ITALY

[6] MAX PLANCK INST ASTRON, D-69117 HEIDELBERG, GERMANY

来源：

ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES | 1997年 / 121卷 / 03期

关键词：

galaxies; fundamental parameters; photometry; infrared; clusters; Virgo cluster;

D O I：

10.1051/aas:1997126

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Near Infrared (K' band) surface photometry has been obtained for 102 (88 late-type) Virgo cluster galaxies. A subset of 20 galaxies was also imaged in the H band. Magnitudes and diameters within the 21.5 and 22.0 mag arcsec(-2) isophote, concentration indices and total H and K' magnitudes are derived. Basic statistical properties of a complete sample of spiral galaxies spanning the range 6.3 < K'(T) < 13.5 are given.(1)

引用

页码：507 / 551

页数：45

共 35 条

[1] INFRARED LUMINOSITY-H I VELOCITY-WIDTH RELATION AND ITS APPLICATION TO THE DISTANCE SCALE [J].