1.65 mu m (H-band) surface photometry of galaxies .2. Observations of 297 galaxies with the TIRGO 1.5 m telescope

被引：34

作者：

Gavazzi, G

Pierini, D

Baffa, C

Lisi, F

Hunt, LK

Randone, I

Boselli, A

机构：

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

[2] OSSERV ASTROFIS ARCETRI,I-50125 FLORENCE,ITALY

[3] CAISMI,I-50125 FLORENCE,ITALY

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

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

来源：

ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES | 1996年 / 120卷 / 03期

关键词：

galaxies; fundamental parameters; photometry; infrared;

D O I：

10.1051/aas:1996309

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present near-infrared H-band (1.65 mu m) surface photometry of 297 galaxies (mostly) in the Coma Supercluster obtained with the Arcetri NICMOS3 camera, ARNICA, mounted on the Gornergrat Infrared Telescope. Magnitudes and diameters within the 21.5 mag arcsec(-2) isophote, concentration indices, and total H magnitudes are derived. Combining these observations with those obtained similarly using the Calar Alto telescopes (Paper I) we find a strong positive correlation between the near-infrared concentration index and the galaxy H-band luminosity, and we analyze the consequent dependence of near-infrared growth-curves on H-band luminosity.

引用

页码：521 / 578

页数：58

共 35 条

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