An Overview of The H I Nearby Galaxy Survey (THINGS)

被引：0
作者：
de Blok, W. J. G. [1 ]
Walter, F. [2 ]
Brinks, E. [3 ]
Bigiel, F. [2 ]
Bagetakos, I. [3 ]
Leroy, A. [2 ]
Oh, S-H [4 ]
Portas, A. [3 ]
Rich, J. W. [4 ]
Tamburro, D. [2 ]
Trachternach, C. [5 ]
Usero, A. [3 ]
Zwaan, M. [6 ]
机构：
[1] Univ Cape Town, Dept Astron, ZA-7700 Rondebosch, South Africa
[2] Max Planck Inst Astron, Heidelberg, Germany
[3] Univ Hertfordshire, Ctr Astrophys Res, Hatfield AL10 9AB, Herts, England
[4] RSAA, Mt Stromlo Observ, Stromlo, Australia
[5] Ruhr Univ Bochum, Astron Inst, Bochum, Germany
[6] ESO, Garching, Germany
来源：
LOW-FREQUENCY RADIO UNIVERSE: AN EVENT COMMEMORATING THE BIRTH CENTENARY OF DR. HOMI J. BHABHA | 2009年 / 407卷
关键词：
STAR-FORMATION; NONCIRCULAR MOTIONS;
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The H I Nearby Galaxy Survey (THINGS) is a high spectral (<= 5.2 km s(-1)) and spatial (similar to 6 '') resolution survey of H (I) emission in 34 nearby galaxies obtained using the NRAO Very Large Array (VLA). The overarching scientific goal of THINGS is to investigate fundamental characteristics of the interstellar medium (ISM) related to galaxy morphology, star formation and mass distribution across the Hubble sequence. Here we summarize some of the recent results obtained with THINGS.
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页码：88 / +
页数：2
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