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Submillimeter Galaxies as Progenitors of Compact Quiescent Galaxies
Astrophysical Journal, 782 (2014), 2; 68. https://doi.org/10.1088/0004-637X/782/2/68
Toft, S.; Smolčić, Vernesa; Magnelli, B.; Karim, A.; Zirm, A.; Michalowski, M.; Capak, P.; Sheth, K.; Schawinski, K.; Krogager, J.-K.; Wuyts, S.; Sanders, D.; Man, A. W. S.; Lutz, D.; Staguhn, J.; Berta, S.; Mccracken, H.; Krpan, J.; Riechers, D. Više autora...

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Institucijski repozitorij: Repozitorij Prirodoslovno-matematičkog fakulteta

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Toft, S., Smolčić, V., Magnelli, B., Karim, A., Zirm, A., Michalowski, M. ... Riechers, D. (2014). Submillimeter Galaxies as Progenitors of Compact Quiescent Galaxies. Astrophysical Journal, 782. (2). doi: 10.1088/0004-637X/782/2/68

Toft, S., et al. "Submillimeter Galaxies as Progenitors of Compact Quiescent Galaxies." Astrophysical Journal, vol. 782, br. 2, 2014. https://doi.org/10.1088/0004-637X/782/2/68

Toft, S., Vernesa Smolčić, B. Magnelli, A. Karim, A. Zirm, M. Michalowski, P. Capak, et al. "Submillimeter Galaxies as Progenitors of Compact Quiescent Galaxies." Astrophysical Journal 782, br. 2 (2014). https://doi.org/10.1088/0004-637X/782/2/68

Toft, S., et al. (2014) 'Submillimeter Galaxies as Progenitors of Compact Quiescent Galaxies', Astrophysical Journal, 782(2). doi: 10.1088/0004-637X/782/2/68

Toft S, Smolčić V, Magnelli B, Karim A, Zirm A, Michalowski M, i sur.. Submillimeter Galaxies as Progenitors of Compact Quiescent Galaxies. Astrophysical Journal [Internet]. 2014. [pristupljeno 28.03.2025.];782(2). doi: 10.1088/0004-637X/782/2/68

S. Toft, et al., "Submillimeter Galaxies as Progenitors of Compact Quiescent Galaxies", Astrophysical Journal, vol. 782, br. 2, 2014. [Online]. Dostupno na: https://urn.nsk.hr/urn:nbn:hr:217:986897. [Citirano: 28.03.2025.]

Za citiranje koristite ovu mrežnu adresu: https://urn.nsk.hr/urn:nbn:hr:217:986897
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Naslov (engleski)Submillimeter Galaxies as Progenitors of Compact Quiescent Galaxies
AutorS. Toft
AutorVernesa Smolčić
AutorB. Magnelli
AutorA. Karim
AutorA. Zirm
AutorM. Michalowski
AutorP. Capak
AutorK. Sheth
AutorK. Schawinski
AutorJ.-K. Krogager
AutorS. Wuyts
AutorD. Sanders
AutorA. W. S. Man
AutorD. Lutz
AutorJ. Staguhn
AutorS. Berta
AutorH. Mccracken
AutorJ. Krpan
AutorD. Riechers
Autorova ustanovaSveučilište u Zagrebu
Prirodoslovno-matematički fakultet
(Fizički odsjek)
Znanstveno / umjetničko
područje, polje i grana		PRIRODNE ZNANOSTI
Fizika
Sažetak (engleski)
Three billion years after the big bang (at redshift z = 2), half of the most massive galaxies were already old, quiescent systems with little to no residual star formation and extremely compact with stellar mass densities at least an order of magnitude larger than in low-redshift ellipticals, their descendants. Little is known about how they formed, but their evolved, dense stellar populations suggest formation within intense, compact starbursts 1-2 Gyr earlier (at 3 < z < 6). Simulations... Više show that gas-rich major mergers can give rise to such starbursts, which produce dense remnants. Submillimeter-selected galaxies (SMGs) are prime examples of intense, gas-rich starbursts. With a new, representative spectroscopic sample of compact, quiescent galaxies at z = 2 and a statistically well- understood sample of SMGs, we show that z = 3-6 SMGs are consistent with being the progenitors of z = 2 quiescent galaxies, matching their formation redshifts and their distributions of sizes, stellar masses, and internal velocities. Assuming an evolutionary connection, their space densities also match if the mean duty cycle of SMG starbursts is 42^{; ; +40}; ; _{; ; -29}; ; Myr (consistent with independent estimates), which indicates that the bulk of stars in these massive galaxies were formed in a major, early surge of star formation. These results suggest a coherent picture of the formation history of the most massive galaxies in the universe, from their initial burst of violent star formation through their appearance as high stellar- density galaxy cores and to their ultimate fate as giant ellipticals. Sakrij dio sažetka
Ključne riječi (engleski)
Jezikengleski
Vrsta publikacijeZnanstveni rad - Izvorni znanstveni rad
Status objaveObjavljen
Vrsta recenzijeRecenziran - međunarodna recenzija
Verzija publikacijeObjavljena verzija rada (izdavačev PDF)
Naslov časopisaAstrophysical Journal
Brojčani podacivol. 782, br. 2, 68
p-ISSN0004-637X
e-ISSN1538-4357
DOIhttps://doi.org/10.1088/0004-637X/782/2/68
URN:NBNurn:nbn:hr:217:986897
Datum objave publikacije2014
URL dokumentahttps://iopscience.iop.org/article/10.1088/0004-637X/782/2/68
Vrsta resursaTekst
Prava pristupaOtvoreni pristup
Uvjeti korištenjaIkona licence Zaštićeno autorskim pravom.
Javna napomenaCopyright (2014). The American Astronomical Society. All rights reserved. Received 2013 September 4; accepted 2013 October 31; published 2014 January 29.
Datum i vrijeme pohrane2019-11-29 16:37:55
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