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• W3106157066 endingPage "A97" @default.
• W3106157066 startingPage "A97" @default.
• W3106157066 abstract "We studied the global characteristics of dust emission in a large sample of emission-line star-forming galaxies. The sample consists of two subsamples. One subsample (SDSS sample) includes ~4000 compact star-forming galaxies from the Sloan Digital Sky Survey (SDSS), which were also detected in all four bands at 3.4 μm, 4.6 μm, 12 μm, and 22 μm of the WISE all-sky survey. The second subsample (Herschel sample) is a sample of 28 compact star-forming galaxies observed with Herschel in the FIR range. Data of the Herschel sample were supplemented by the photometric data from the Spitzer observations, GALaxy Evolution Explorer (GALEX) survey, SDSS, Wide-Field Infrared Survey Explorer (WISE), Two Micron All Sky Survey (2MASS), NRAO VLA Sky Survey (NVSS), and Faint Images of the Radio Sky at Twenty-cm (FIRST) survey, as well as optical and Spitzer spectra and data in submm and radio ranges. It is found that warm dust luminosities of galaxies from the SDSS sample and cold and warm dust luminosities of galaxies from the Herschel sample are strongly correlated with Hβ luminosities, which implies that one of the main sources of dust heating in star-forming galaxies is ionising UV radiation of young stars. Likely, a significant fraction of dust is located inside H ii and surrounding regions. We found tight correlations between masses of cold and warm dust, again implying the same source of dust heating. Using the relation between warm and cold dust masses for estimating the total dust mass in star-forming galaxies with an accuracy better than ~0.5 dex is proposed. On the other hand, it is shown for both samples that dust temperatures do not depend on the metallicities. The dust-to-neutral gas mass ratio strongly declines with decreasing metallicity, similar to that found in other studies of local emission-line galaxies, high-redshift gamma-ray burst hosts, and damped Ly-α absorbers. On the other hand, the dust-to-ionised gas mass ratio is about one hundred times as high implying that most of dust is located in the neutral gas. It is found that thermal free-free emission of ionised gas in compact star-forming galaxies is important in the submm and mm ranges, and it might be responsible for the submm emission excess. This effect is stronger in galaxies with lower metallicities and is also positively affected by an increased star-formation rate." @default.
• W3106157066 created "2020-11-23" @default.
• W3106157066 creator A5027080885 @default.
• W3106157066 creator A5029044253 @default.
• W3106157066 creator A5046193446 @default.
• W3106157066 creator A5063027126 @default.
• W3106157066 creator A5077156611 @default.
• W3106157066 date "2014-10-01" @default.
• W3106157066 modified "2023-10-14" @default.
• W3106157066 title "Dust emission in star-forming dwarf galaxies: General properties and the nature of the submm excess" @default.
• W3106157066 cites W1648312556 @default.
• W3106157066 cites W1964925572 @default.
• W3106157066 cites W1966589519 @default.
• W3106157066 cites W1966667130 @default.
• W3106157066 cites W1973105125 @default.
• W3106157066 cites W1974347469 @default.
• W3106157066 cites W1980047882 @default.
• W3106157066 cites W1980124829 @default.
• W3106157066 cites W1980193943 @default.
• W3106157066 cites W1982889622 @default.
• W3106157066 cites W1992168233 @default.
• W3106157066 cites W1994463388 @default.
• W3106157066 cites W1996537612 @default.
• W3106157066 cites W1997644455 @default.
• W3106157066 cites W2000020331 @default.
• W3106157066 cites W2001356143 @default.
• W3106157066 cites W2004311301 @default.
• W3106157066 cites W2005969891 @default.
• W3106157066 cites W2009895254 @default.
• W3106157066 cites W2010633418 @default.
• W3106157066 cites W2013366229 @default.
• W3106157066 cites W2015267403 @default.
• W3106157066 cites W2017160063 @default.
• W3106157066 cites W2018657673 @default.
• W3106157066 cites W2022990317 @default.
• W3106157066 cites W2024716567 @default.
• W3106157066 cites W2025235333 @default.
• W3106157066 cites W2027204528 @default.
• W3106157066 cites W2034608771 @default.
• W3106157066 cites W2035048769 @default.
• W3106157066 cites W2039847154 @default.
• W3106157066 cites W2041561966 @default.
• W3106157066 cites W204192878 @default.
• W3106157066 cites W2042470708 @default.
• W3106157066 cites W2042921214 @default.
• W3106157066 cites W2045531469 @default.
• W3106157066 cites W2049866079 @default.
• W3106157066 cites W2051142510 @default.
• W3106157066 cites W2051546265 @default.
• W3106157066 cites W2052305773 @default.
• W3106157066 cites W2052937506 @default.
• W3106157066 cites W2055004653 @default.
• W3106157066 cites W2056076677 @default.
• W3106157066 cites W2063869643 @default.
• W3106157066 cites W2065390672 @default.
• W3106157066 cites W2066492340 @default.
• W3106157066 cites W2067813516 @default.
• W3106157066 cites W2068928940 @default.
• W3106157066 cites W2070005169 @default.
• W3106157066 cites W2075029364 @default.
• W3106157066 cites W2075110254 @default.
• W3106157066 cites W2078007854 @default.
• W3106157066 cites W2079055653 @default.
• W3106157066 cites W2081120960 @default.
• W3106157066 cites W2084852342 @default.
• W3106157066 cites W2090400051 @default.
• W3106157066 cites W2090992720 @default.
• W3106157066 cites W2097701558 @default.
• W3106157066 cites W2102097999 @default.
• W3106157066 cites W2105983108 @default.
• W3106157066 cites W2107959100 @default.
• W3106157066 cites W2114395264 @default.
• W3106157066 cites W2114860619 @default.
• W3106157066 cites W2118435754 @default.
• W3106157066 cites W2119776555 @default.
• W3106157066 cites W2119950119 @default.
• W3106157066 cites W2124199755 @default.
• W3106157066 cites W2127014496 @default.
• W3106157066 cites W2130606217 @default.
• W3106157066 cites W2134050590 @default.
• W3106157066 cites W2134273479 @default.
• W3106157066 cites W2136607433 @default.
• W3106157066 cites W2142220522 @default.
• W3106157066 cites W2149476548 @default.
• W3106157066 cites W2150531016 @default.
• W3106157066 cites W2153107905 @default.
• W3106157066 cites W2155297672 @default.
• W3106157066 cites W2159496414 @default.
• W3106157066 cites W2167635287 @default.
• W3106157066 cites W2171417273 @default.
• W3106157066 cites W2493738155 @default.
• W3106157066 cites W2761061330 @default.
• W3106157066 cites W3042750865 @default.
• W3106157066 cites W3097992367 @default.
• W3106157066 cites W3098003348 @default.
• W3106157066 cites W3098186308 @default.
• W3106157066 cites W3098245571 @default.
• W3106157066 cites W3098676073 @default.

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