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Cospatial Star Formation and Supermassive Black Hole Growth in z ~ 3 Galaxies: Evidence for In Situ Co-evolution
Astrophysical Journal Letters, 854 (2018), 1; L4. https://doi.org/10.3847/2041-8213/aaa9b3
Rujopakarn, W.; Nyland, K.; Rieke, G. H.; Barro, G.; Elbaz, D.; Ivison, R. J.; Jagannathan, P.; Silverman, J. D.; Smolčić, Vernesa; Wang, T.

Institucijski repozitorij: Repozitorij Prirodoslovno-matematičkog fakulteta

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Rujopakarn, W., Nyland, K., Rieke, G. H., Barro, G., Elbaz, D., Ivison, R. J. ... Wang, T. (2018). Cospatial Star Formation and Supermassive Black Hole Growth in z ~ 3 Galaxies: Evidence for In Situ Co-evolution. Astrophysical Journal Letters, 854. (1). doi: 10.3847/2041-8213/aaa9b3

Rujopakarn, W., et al. "Cospatial Star Formation and Supermassive Black Hole Growth in z ~ 3 Galaxies: Evidence for In Situ Co-evolution." Astrophysical Journal Letters, vol. 854, br. 1, 2018. https://doi.org/10.3847/2041-8213/aaa9b3

Rujopakarn, W., K. Nyland, G. H. Rieke, G. Barro, D. Elbaz, R. J. Ivison, P. Jagannathan, J. D. Silverman, Vernesa Smolčić i T. Wang. "Cospatial Star Formation and Supermassive Black Hole Growth in z ~ 3 Galaxies: Evidence for In Situ Co-evolution." Astrophysical Journal Letters 854, br. 1 (2018). https://doi.org/10.3847/2041-8213/aaa9b3

Rujopakarn, W., et al. (2018) 'Cospatial Star Formation and Supermassive Black Hole Growth in z ~ 3 Galaxies: Evidence for In Situ Co-evolution', Astrophysical Journal Letters, 854(1). doi: 10.3847/2041-8213/aaa9b3

Rujopakarn W, Nyland K, Rieke GH, Barro G, Elbaz D, Ivison RJ, i sur.. Cospatial Star Formation and Supermassive Black Hole Growth in z ~ 3 Galaxies: Evidence for In Situ Co-evolution. Astrophysical Journal Letters [Internet]. 2018. [pristupljeno 22.11.2024.];854(1). doi: 10.3847/2041-8213/aaa9b3

W. Rujopakarn, et al., "Cospatial Star Formation and Supermassive Black Hole Growth in z ~ 3 Galaxies: Evidence for In Situ Co-evolution", Astrophysical Journal Letters, vol. 854, br. 1, 2018. [Online]. Dostupno na: https://urn.nsk.hr/urn:nbn:hr:217:485433. [Citirano: 22.11.2024.]

Za citiranje koristite ovu mrežnu adresu: https://urn.nsk.hr/urn:nbn:hr:217:485433
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Naslov (engleski)Cospatial Star Formation and Supermassive Black Hole Growth in z ~ 3 Galaxies: Evidence for In Situ Co-evolution
AutorW. Rujopakarn
AutorK. Nyland
AutorG. H. Rieke
AutorG. Barro
AutorD. Elbaz
AutorR. J. Ivison
AutorP. Jagannathan
AutorJ. D. Silverman
AutorVernesa Smolčić
AutorT. Wang
Autorova ustanovaSveučilište u Zagrebu
Prirodoslovno-matematički fakultet
(Fizički odsjek)
Znanstveno / umjetničko
područje, polje i grana		PRIRODNE ZNANOSTI
Fizika
Astronomija i astrofizika
Sažetak (engleski)
We present a sub-kiloparsec localization of the sites of supermassive black hole (SMBH) growth in three active galactic nuclei (AGNs) at z ~ 3 in relation to the regions of intense star formation in their hosts. These AGNs are selected from Karl G. Jansky Very Large Array (VLA) and Atacama Large Millimeter/submillimeter Array (ALMA) observations in the Hubble Ultra-Deep Field and COSMOS, with the centimetric radio emission tracing both star formation and AGN, and the sub/millimeter emission by dust tracing nearly pure star formation. We require radio emission to be $\geqslant 5\times $ more luminous than the level associated with the sub/millimeter star formation to ensure that the radio emission is AGN-dominated, thereby allowing localization of the AGN and star formation independently. In all three galaxies, the AGNs are located within the compact regions of gas- rich, heavily obscured, intense nuclear star formation, with R e = 0.4–1.1 kpc and average star formation rates of sime100–1200 M ⊙ yr−1. If the current episode of star formation continues at such a rate over the stellar mass doubling time of their hosts, sime0.2 Gyr, the newly formed stellar mass will be of the order of 1011 M ⊙ within the central kiloparsec region, concurrently and cospatially with significant growth of the SMBH. This is consistent with a picture of in situ galactic bulge and SMBH formation. This work demonstrates the unique complementarity of VLA and ALMA observations to unambiguously pinpoint the locations of AGNs and star formation down to sime30 mas, corresponding to sime230 pc at z = 3.
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 Letters
Brojčani podacivol. 854, br. 1, L4
p-ISSN2041-8205
DOIhttps://doi.org/10.3847/2041-8213/aaa9b3
URN:NBNurn:nbn:hr:217:485433
Datum objave publikacije2018
URL dokumentahttps://iopscience.iop.org/article/10.3847/2041-8213/aaa9b3
Vrsta resursaTekst
Prava pristupaOtvoreni pristup
Uvjeti korištenjaIkona licence Zaštićeno autorskim pravom.
Javna napomena© 2018. The American Astronomical Society. Received 2017 December 7; accepted 2018 January 21; published 2018 February 7.
Datum i vrijeme pohrane2020-03-01 16:38:58