prikaz prve stranice dokumenta Evolution of the dust emission of massive galaxies up to z = 4 and constraints on their dominant mode of star formation
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Evolution of the dust emission of massive galaxies up to z = 4 and constraints on their dominant mode of star formation
Astronomy and Astrophysics, 573 (2015); 113. https://doi.org/10.1051/0004-6361/201425031
Béthermin, Matthieu; Daddi, Emanuele; Magdis, Georgios; Lagos, Claudia; Sargent, Mark; Albrecht, Marcus; Aussel, Hervé; Bertoldi, Frank; Buat, Véronique; Galametz, Maud; Heinis, Sébastien; Ilbert, Olivier; Karim, Alexander; Koekemoer, Anton; Lacey, Cedric; Le Floc'h, Emeric; Navarrete, Felipe; Pannella, Maurilio; Schreiber, Corentin; Smolčić, Vernesa; Symeonidis, Myrto; Viero, Marco Više autora...

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Béthermin, M., Daddi, E., Magdis, G., Lagos, C., Sargent, M., Albrecht, M. ... Viero, M. (2015). Evolution of the dust emission of massive galaxies up to z = 4 and constraints on their dominant mode of star formation. Astronomy and Astrophysics, 573.. doi: 10.1051/0004-6361/201425031

Béthermin, Matthieu, et al. "Evolution of the dust emission of massive galaxies up to z = 4 and constraints on their dominant mode of star formation." Astronomy and Astrophysics, vol. 573, 2015. https://doi.org/10.1051/0004-6361/201425031

Béthermin, Matthieu, Emanuele Daddi, Georgios Magdis, Claudia Lagos, Mark Sargent, Marcus Albrecht, Hervé Aussel, et al. "Evolution of the dust emission of massive galaxies up to z = 4 and constraints on their dominant mode of star formation." Astronomy and Astrophysics 573 (2015). https://doi.org/10.1051/0004-6361/201425031

Béthermin, M., et al. (2015) 'Evolution of the dust emission of massive galaxies up to z = 4 and constraints on their dominant mode of star formation', Astronomy and Astrophysics, 573. doi: 10.1051/0004-6361/201425031

Béthermin M, Daddi E, Magdis G, Lagos C, Sargent M, Albrecht M, i sur.. Evolution of the dust emission of massive galaxies up to z = 4 and constraints on their dominant mode of star formation. Astronomy and Astrophysics [Internet]. 2015. [pristupljeno 26.10.2024.];573. doi: 10.1051/0004-6361/201425031

M. Béthermin, et al., "Evolution of the dust emission of massive galaxies up to z = 4 and constraints on their dominant mode of star formation", Astronomy and Astrophysics, vol. 573, 2015. [Online]. Dostupno na: https://urn.nsk.hr/urn:nbn:hr:217:943144. [Citirano: 26.10.2024.]

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Naslov (engleski)Evolution of the dust emission of massive galaxies up to z = 4 and constraints on their dominant mode of star formation
AutorMatthieu Béthermin
AutorEmanuele Daddi
AutorGeorgios Magdis
AutorClaudia Lagos
AutorMark Sargent
AutorMarcus Albrecht
AutorHervé Aussel
AutorFrank Bertoldi
AutorVéronique Buat
AutorMaud Galametz
AutorSébastien Heinis
AutorOlivier Ilbert
AutorAlexander Karim
AutorAnton Koekemoer
AutorCedric Lacey
AutorEmeric Le Floc'h
AutorFelipe Navarrete
AutorMaurilio Pannella
AutorCorentin Schreiber
AutorVernesa Smolčić
AutorMyrto Symeonidis
AutorMarco Viero
Autorova ustanovaSveučilište u Zagrebu
Prirodoslovno-matematički fakultet
(Fizički odsjek)
Znanstveno / umjetničko
područje, polje i grana		PRIRODNE ZNANOSTI
Fizika
Astronomija i astrofizika
Sažetak (engleski)
We aim to measure the average dust and molecular gas content of massive star-forming galaxies (>3 × 10^(10)M_⊙) up to z = 4 in the COSMOS field to determine if the intense star formation observed at high redshift is induced by major mergers or is caused by large gas reservoirs. Firstly, we measured the evolution of the average spectral energy distributions as a function of redshift using a stacking analysis of Spitzer, Herschel, LABOCA, and AzTEC data for two samples of galaxies: normal star-forming objects and strong starbursts, as defined by their distance to the main sequence. We found that the mean intensity of the radiation field ⟨ U ⟩ heating the dust (strongly correlated with dust temperature) increases with increasing redshift up to z = 4 in main-sequence galaxies. We can reproduce this evolution with simple models that account for the decrease in the gas metallicity with redshift. No evolution of ⟨ U ⟩ with redshift is found in strong starbursts. We then deduced the evolution of the molecular gas fraction (defined here as M_(mol)/(M_(mol)+M_⋆)) with redshift and found a similar, steeply increasing trend for both samples. At z ~ 4, this fraction reaches ~60%. The average position of the main-sequence galaxies is on the locus of the local, normal star-forming disks in the integrated Schmidt-Kennicutt diagram (star formation rate versus mass of molecular gas), suggesting that the bulk of the star formation up to z = 4 is dominated by secular processes.
Ključne riječi (engleski)
Jezikengleski
Vrsta publikacijeZnanstveni rad - Izvorni znanstveni rad
Status objaveObjavljen
Vrsta recenzijeRecenziran - međunarodna recenzija
Verzija publikacijeObjavljena verzija rada (izdavačev PDF)
Naslov časopisaAstronomy and Astrophysics
Brojčani podacivol. 573, 113
p-ISSN0004-6361
DOIhttps://doi.org/10.1051/0004-6361/201425031
URN:NBNurn:nbn:hr:217:943144
Datum objave publikacije2015
URL dokumentahttp://dx.doi.org/10.1051/0004-6361/201425031
Vrsta resursaTekst
Prava pristupaOtvoreni pristup
Uvjeti korištenjaIkona licence Zaštićeno autorskim pravom.
Javna napomena© 2015 ESO. Received: 19 September 2014. Accepted: 11 November 2014. Published online 07 January 2015.
Datum i vrijeme pohrane2019-12-30 12:11:12