Dust and gas in star-forming complexes in NGC 3351, NGC 5055, and NGC 5457

IF 0.5 4区物理与天体物理 Q4 ASTRONOMY & ASTROPHYSICS

Open Astronomy Pub Date : 2023-01-01 DOI:10.1515/astro-2022-0219

K. Smirnova, D. Wiebe

引用次数: 0

Abstract

Abstract We present a study of the interstellar medium parameters in star-forming complexes (SFCs) in NGC 3351, NGC 5055, and NGC 5457 galaxies. This study concludes our previous investigations of gas and dust in a number of spiral galaxies. The data for the three galaxies confirm the following. There is a tight correlation between near-infrared and far-infrared luminosities of the extragalactic SFCs. Emission at 8 μm also shows a strong correlation with the carbon monoxide emission. Atomic and molecular gas masses do not show any strong correlation with the corresponding velocity scatters; however, in NGC 5055, we see a hint of the SFC with the largest velocity scatter being located at the galaxy periphery.

查看原文本刊更多论文

NGC 3351、NGC 5055和NGC 5457恒星形成复合体中的尘埃和气体

摘要我们研究了NGC3351、NGC5055和NGC5457星系中恒星形成复合体（SFCs）的星际介质参数。这项研究结束了我们之前对许多螺旋星系中气体和尘埃的研究。这三个星系的数据证实了以下几点。河外SFCs的近红外和远红外亮度之间存在着紧密的相关性。8μm的排放量也与一氧化碳排放量有很强的相关性。原子和分子气体质量与相应的速度散射没有显示出任何强相关性；然而，在NGC 5055中，我们看到了SFC的暗示，其最大的速度散射位于星系外围。

本文章由计算机程序翻译，如有差异，请以英文原文为准。

求助全文

约1分钟内获得全文求助全文

来源期刊

Open Astronomy Physics and Astronomy-Astronomy and Astrophysics

CiteScore

1.30

自引率

14.30%

发文量

审稿时长

16 weeks

期刊介绍： The journal disseminates research in both observational and theoretical astronomy, astrophysics, solar physics, cosmology, galactic and extragalactic astronomy, high energy particles physics, planetary science, space science and astronomy-related astrobiology, presenting as well the surveys dedicated to astronomical history and education.