Radio emission at 1.4 GHz from luminous compact galaxies

被引：3

作者：

Parnovsky, S. L. ^{[1
]}

Izotova, I. Y. ^{[1
]}

机构：

[1] Taras Shevchenko Kyiv Natl Univ, Astron Observ, UA-04053 Kiev, Ukraine

来源：

ASTRONOMISCHE NACHRICHTEN | 2015年 / 336卷 / 03期

基金：

美国国家航空航天局; 美国国家科学基金会;

关键词：

galaxies: starburst; galaxies: star formation; methods: statistical; radio continuum: galaxies; STAR-FORMATION RATES; DWARF GALAXIES; LINE GALAXIES; H-ALPHA; SKY; LUMINOSITIES; ULTRAVIOLET; EXTINCTION;

D O I：

10.1002/asna.201412163

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We analyse the properties of the 1.4 GHz continuum emission in 52 star-forming compact luminous galaxies (LCGs). The fluxes of the 1.4 GHz thermal (free-free) component are derived from the extinction- and aperture-corrected fluxes of the H emission line. The fraction of the thermal 1.4 GHz emission is shown tobe in the range of 2-52 % with a median value of about 15-17 %, and its distribution is close to a log-normal one. Both the thermal and non-thermal radio continuum luminosities are shown to be proportional to the masses of the young stellar population of the LCGs. We discuss the approximation of the ratio of the 1.4 GHz luminosity-to-the mass of the young stellar population as a function of starburst age. The derived approximation is shown to be similar but less clearly defined compared to ones obtained previously for LCGs from their H and UV continuum luminosities. ((c) 2015 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim)

引用

页码：276 / 283

页数：8

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