VELOCITY-RESOLVED INFRARED RECOMBINATION-LINE SPECTROSCOPY OF NGC-253

被引：8

作者：

PUXLEY, PJ ^{[1
]}

BRAND, PWJL ^{[1
]}

机构：

[1] UNIV EDINBURGH,INST ASTRON,EDINBURGH EH9 3HJ,MIDLOTHIAN,SCOTLAND

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1995年 / 274卷 / 04期

关键词：

DUST; EXTINCTION; GALAXIES; INDIVIDUAL; NGC; 253; KINEMATICS AND DYNAMICS; STARBURST; INFRARED;

D O I：

10.1093/mnras/274.1.L77

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Observations at high spectral resolution of the Br gamma hydrogen recombination line are presented for the central 25 arcsec of the starburst galaxy NGC 253. The rotation curve derived from these data shows solid body rotation consistent with recent interferometric CO measurements but not with rotation curves derived from optical emission lines. This discrepancy is most likely due to heavy dust extinction along the line of sight causing the optical lines to underestimate the radial velocity. This dust must be located foreground to the region undergoing solid body rotation.

引用

页码：L77 / L80

页数：4

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