prikaz prve stranice dokumenta Probing star formation and ISM properties using galaxy disk inclination. I. Evolution in disk opacity since z ~ 0.7
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Probing star formation and ISM properties using galaxy disk inclination. I. Evolution in disk opacity since z ~ 0.7
Astronomy and Astrophysics, 615 (2018); A7. https://doi.org/10.1051/0004-6361/201732255
Leslie, S. K.; Sargent, M. T.; Schinnerer, E.; Groves, B.; van der Wel, Arjen; Zamorani, G.; Fudamoto, Y.; Lang, P.; Smolčić, Vernesa

Institucijski repozitorij: Repozitorij Prirodoslovno-matematičkog fakulteta

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Leslie, S. K., Sargent, M. T., Schinnerer, E., Groves, B., van der Wel, A., Zamorani, G. ... Smolčić, V. (2018). Probing star formation and ISM properties using galaxy disk inclination. I. Evolution in disk opacity since z ~ 0.7. Astronomy and Astrophysics, 615.. doi: 10.1051/0004-6361/201732255

Leslie, S. K., et al. "Probing star formation and ISM properties using galaxy disk inclination. I. Evolution in disk opacity since z ~ 0.7." Astronomy and Astrophysics, vol. 615, 2018. https://doi.org/10.1051/0004-6361/201732255

Leslie, S. K., M. T. Sargent, E. Schinnerer, B. Groves, Arjen van der Wel, G. Zamorani, Y. Fudamoto, P. Lang i Vernesa Smolčić. "Probing star formation and ISM properties using galaxy disk inclination. I. Evolution in disk opacity since z ~ 0.7." Astronomy and Astrophysics 615 (2018). https://doi.org/10.1051/0004-6361/201732255

Leslie, S. K., et al. (2018) 'Probing star formation and ISM properties using galaxy disk inclination. I. Evolution in disk opacity since z ~ 0.7', Astronomy and Astrophysics, 615. doi: 10.1051/0004-6361/201732255

Leslie SK, Sargent MT, Schinnerer E, Groves B, van der Wel A, Zamorani G, i sur.. Probing star formation and ISM properties using galaxy disk inclination. I. Evolution in disk opacity since z ~ 0.7. Astronomy and Astrophysics [Internet]. 2018. [pristupljeno 22.11.2024.];615. doi: 10.1051/0004-6361/201732255

S. K. Leslie, et al., "Probing star formation and ISM properties using galaxy disk inclination. I. Evolution in disk opacity since z ~ 0.7", Astronomy and Astrophysics, vol. 615, 2018. [Online]. Dostupno na: https://urn.nsk.hr/urn:nbn:hr:217:656958. [Citirano: 22.11.2024.]

Za citiranje koristite ovu mrežnu adresu: https://urn.nsk.hr/urn:nbn:hr:217:656958
Podaci o radu
Naslov (engleski)Probing star formation and ISM properties using galaxy disk inclination. I. Evolution in disk opacity since z ~ 0.7
AutorS. K. Leslie
AutorM. T. Sargent
AutorE. Schinnerer
AutorB. Groves
AutorArjen van der Wel
AutorG. Zamorani
AutorY. Fudamoto
AutorP. Lang
AutorVernesa Smolčić
MBZ: 336180
Autorova ustanovaSveučilište u Zagrebu
Prirodoslovno-matematički fakultet
(Fizički odsjek)
Znanstveno / umjetničko
područje, polje i grana		PRIRODNE ZNANOSTI
Fizika
Astronomija i astrofizika
Sažetak (engleski)
Disk galaxies at intermediate redshift (z ~ 0:7) have been found in previous work to display more optically thick behaviour than their local counterparts in the rest-frame B- band surface brightness, suggesting an evolution in dust properties over the past ~6 Gyr. We compare the measured luminosities of face-on and edge-on star-forming galaxies at different wavelengths (Ultraviolet (UV), midinfrared (MIR), far-infrared (FIR), and radio) for two well-matched samples of disk- dominated galaxies: a local Sloan Digital Sky Survey (SDSS)-selected sample at z ~ 0:07 and a sample of disks at z ~ 0:7 drawn from Cosmic Evolution Survey (COSMOS). We have derived correction factors to account for the inclination dependence of the parameters used for sample selection. We find that typical galaxies are transparent at MIR wavelengths at both redshifts, and that the FIR and radio emission is also transparent as expected. However, reduced sensitivity at these wavelengths limits our analysis ; we cannot rule out opacity in the FIR or radio. Ultra-violet attenuation has increased between z ~ 0 and z ~ 0:7, with the z ~ 0:7 sample being a factor of ~3.4 more attenuated. The larger UV attenuation at z ~ 0:7 can be explained by more clumpy dust around nascent star-forming regions. There is good agreement between the fitted evolution of the normalisation of the SFR_UV versus 1 − cos(i) trend (interpreted as the clumpiness fraction) and the molecular gas fraction/dust fraction evolution of galaxies found out to z < 1.
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. 615, A7
p-ISSN0004-6361
e-ISSN1432-0746
DOIhttps://doi.org/10.1051/0004-6361/201732255
URN:NBNurn:nbn:hr:217:656958
Datum objave publikacije2018
URL dokumentahttps://www.aanda.org/articles/aa/abs/2018/07/aa32255-17/aa32255-17.html
Vrsta resursaTekst
Prava pristupaOtvoreni pristup
Uvjeti korištenjaIkona licence Zaštićeno autorskim pravom.
Javna napomena© ESO 2018. Received 7 November 2017. Accepted 22 December 2017. Published online 03 July 2018.
Datum i vrijeme pohrane2020-03-01 12:08:14