The Tully-Fisher relation for flat galaxies

被引：7
|
作者：
Makarov, D. I. [1 ]
Zaitseva, N. A. [2 ]
Bizyaev, D. V. [2 ,3 ,4 ]
机构：
[1] RAS, Special Astrophys Observ, Nizhnii Arkhyz 369167, Karachai Circas, Russia
[2] Moscow MV Lomonosov State Univ, Sternberg Astron Inst, Univ Skij Pr 13, Moscow 119991, Russia
[3] Apache Point Observ, Sunspot, NM 88349 USA
[4] New Mexico State Univ, Sunspot, NM 88349 USA
来源：
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2018年 / 479卷 / 03期
基金：
俄罗斯科学基金会;
关键词：
galaxies: fundamental parameters; galaxies: general; EDGE-ON GALAXIES; EXTRAGALACTIC DISTANCE DATABASE; VENATICI-I CLOUD; STELLAR DISKS; DWARF GALAXIES; COSMIC FLOWS; BULK MOTION; DARK HALO; SPIRAL GALAXIES; FGC GALAXIES;
D O I：
10.1093/mnras/sty1629
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We construct a multiparametric Tully-Fisher (TF) relation for a large sample of edge-on galaxies from the Revised Flat Galaxy Catalog using HI data from the Extragalactic Distance Database and parameters from the edge-on disc galaxies catalogue. We incorporate a variety of additional parameters including structural parameters of edge-on galaxies in different bandpasses. Besides the rotation curve maximum, only the HI-to-optical luminosity ratio and optical colours play a statistically significant role in the multiparametric TF relation. We are able to decrease the standard deviation of the multiparametric TF relation down to 0.32 mag, which is at the level of best modern samples of galaxies used for studies of the matter motion in the Universe via the TF relation.
引用
收藏
页码：3373 / 3380
页数：8
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