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

Standard

Dust and gas in star-forming complexes in NGC 3351, NGC 5055, and NGC 5457. / Smirnova, Ksenia ildarovna; Wiebe, Dmitri siegfriedovich.
In: Open Astronomy, Vol. 32, No. 1, 20220219, 01.01.2023.

Research output: Contribution to journal › Article › peer-review

BibTeX

@article{08c24501c9d54930bfdf9e16877f913a,

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

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.",

author = "Smirnova, {Ksenia ildarovna} and Wiebe, {Dmitri siegfriedovich}",

note = "Funding information : K. Smirnova was supported by the Russian Ministry of Science and Higher Education via state assignment FEUZ-2020-0038. D. Wiebe was supported by the Russian Science Foundation (Grant 21-12-00373).",

year = "2023",

month = jan,

day = "1",

doi = "10.1515/astro-2022-0219",

language = "English",

volume = "32",

journal = "Open Astronomy",

issn = "2543-6376",

publisher = "De Gruyter Open Ltd.",

number = "1",

}

RIS

TY - JOUR

T1 - Dust and gas in star-forming complexes in NGC 3351, NGC 5055, and NGC 5457

AU - Smirnova, Ksenia ildarovna

AU - Wiebe, Dmitri siegfriedovich

N1 - Funding information : K. Smirnova was supported by the Russian Ministry of Science and Higher Education via state assignment FEUZ-2020-0038. D. Wiebe was supported by the Russian Science Foundation (Grant 21-12-00373).

PY - 2023/1/1

Y1 - 2023/1/1

N2 - 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.

AB - 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.

UR - http://www.scopus.com/inward/record.url?partnerID=8YFLogxK&scp=85156214956

UR - https://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=tsmetrics&SrcApp=tsm_test&DestApp=WOS_CPL&DestLinkType=FullRecord&KeyUT=000978718100001

U2 - 10.1515/astro-2022-0219

DO - 10.1515/astro-2022-0219

M3 - Article

VL - 32

JO - Open Astronomy

JF - Open Astronomy

SN - 2543-6376

IS - 1

M1 - 20220219

ER -

ID: 38489702