prikaz prve stranice dokumenta Cospatial Star Formation and Supermassive Black Hole Growth in z ~ 3 Galaxies: Evidence for In Situ Co-evolution
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Scientific paper - Original scientific paper
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.

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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, no. 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 and T. Wang. "Cospatial Star Formation and Supermassive Black Hole Growth in z ~ 3 Galaxies: Evidence for In Situ Co-evolution." Astrophysical Journal Letters 854, no. 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, and sur.. Cospatial Star Formation and Supermassive Black Hole Growth in z ~ 3 Galaxies: Evidence for In Situ Co-evolution. Astrophysical Journal Letters [Internet]. 2018 [cited 2024 August 30];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, no. 1, 2018. [Online]. Available at: https://urn.nsk.hr/urn:nbn:hr:217:485433. [Accessed: 30 August 2024]

Metadata
Title (english)Cospatial Star Formation and Supermassive Black Hole Growth in z ~ 3 Galaxies: Evidence for In Situ Co-evolution
AuthorW. Rujopakarn
AuthorK. Nyland
AuthorG. H. Rieke
AuthorG. Barro
AuthorD. Elbaz
AuthorR. J. Ivison
AuthorP. Jagannathan
AuthorJ. D. Silverman
AuthorVernesa Smolčić
AuthorT. Wang
Author's institutionUniversity of Zagreb
Faculty of Science
(Department of Physics)
Scientific / art field,
discipline and subdiscipline		NATURAL SCIENCES
Physics
Astronomy and Astrophysics
Abstract (english)
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.
Keywords (english)
Languageenglish
Publication typeScientific paper - Original scientific paper
Publication statusPublished
Peer reviewPeer review - international
Publication versionPublished version
Journal titleAstrophysical Journal Letters
Numberingvol. 854, no. 1, L4
p-ISSN2041-8205
DOIhttps://doi.org/10.3847/2041-8213/aaa9b3
URN:NBNurn:nbn:hr:217:485433
Publication2018
Document URLhttps://iopscience.iop.org/article/10.3847/2041-8213/aaa9b3
Type of resourceText
Access conditionsOpen access
Terms of useLicence In copyright icon
Public note© 2018. The American Astronomical Society. Received 2017 December 7; accepted 2018 January 21; published 2018 February 7.
Created on2020-03-01 16:38:58