prikaz prve stranice dokumenta The Ly α, C iv, and He ii nebulae around J1000+0234: a galaxy pair at the centre of a galaxy overdensity at z=4.5
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Scientific paper - Original scientific paper
The Ly α, C iv, and He ii nebulae around J1000+0234: a galaxy pair at the centre of a galaxy overdensity at z=4.5
Monthly Notices of the Royal Astronomical Society, 521 (2023), 2; 2326-2341. https://doi.org/10.1093/mnras/stad594
Jiménez-Andrade, E F; Cantalupo, S; Magnelli, B; Romano-Díaz, E; Gómez-Guijarro, C; Mackenzie, R; Smolčić, Vernesa; Murphy, E; Matthee, J; Toft, S

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Jiménez Andrade, E. F., Cantalupo, S., Magnelli, B., Romano Díaz, E., Gómez Guijarro, C., Mackenzie, R. ... Toft, S. (2023). The Ly α, C iv, and He ii nebulae around J1000+0234: a galaxy pair at the centre of a galaxy overdensity at z=4.5. Monthly Notices of the Royal Astronomical Society, 521. (2), 2326-2341. doi: 10.1093/mnras/stad594

Jiménez Andrade, E F, et al. "The Ly α, C iv, and He ii nebulae around J1000+0234: a galaxy pair at the centre of a galaxy overdensity at z=4.5." Monthly Notices of the Royal Astronomical Society, vol. 521, no. 2, 2023, pp. 2326-2341. https://doi.org/10.1093/mnras/stad594

Jiménez Andrade, E F, S Cantalupo, B Magnelli, E Romano Díaz, C Gómez Guijarro, R Mackenzie, Vernesa Smolčić, E Murphy, J Matthee and S Toft. "The Ly α, C iv, and He ii nebulae around J1000+0234: a galaxy pair at the centre of a galaxy overdensity at z=4.5." Monthly Notices of the Royal Astronomical Society 521, no. 2 (2023): 2326-2341. https://doi.org/10.1093/mnras/stad594

Jiménez Andrade, E. F., et al. (2023) 'The Ly α, C iv, and He ii nebulae around J1000+0234: a galaxy pair at the centre of a galaxy overdensity at z=4.5', Monthly Notices of the Royal Astronomical Society, 521(2), pp. 2326-2341. doi: 10.1093/mnras/stad594

Jiménez Andrade EF, Cantalupo S, Magnelli B, Romano Díaz E, Gómez Guijarro C, Mackenzie R, and sur.. The Ly α, C iv, and He ii nebulae around J1000+0234: a galaxy pair at the centre of a galaxy overdensity at z=4.5. Monthly Notices of the Royal Astronomical Society [Internet]. 2023 May [cited 2024 July 26];521(2):2326-2341. doi: 10.1093/mnras/stad594

E. F. Jiménez Andrade, et al., "The Ly α, C iv, and He ii nebulae around J1000+0234: a galaxy pair at the centre of a galaxy overdensity at z=4.5", Monthly Notices of the Royal Astronomical Society, vol. 521, no. 2, pp. 2326-2341, May 2023. [Online]. Available at: https://urn.nsk.hr/urn:nbn:hr:217:142972. [Accessed: 26 July 2024]

Metadata
Title (english)The Ly α, C iv, and He ii nebulae around J1000+0234: a galaxy pair at the centre of a galaxy overdensity at z=4.5
AuthorE F Jiménez-Andrade
AuthorS Cantalupo
AuthorB Magnelli
AuthorE Romano-Díaz
AuthorC Gómez-Guijarro
AuthorR Mackenzie
AuthorVernesa Smolčić
AuthorE Murphy
AuthorJ Matthee
AuthorS Toft
Author's institutionUniversity of Zagreb
Faculty of Science
(Department of Physics)
Scientific / art field,
discipline and subdiscipline		NATURAL SCIENCES
Physics
Abstract (english)
ABSTRACT Ly α λ1216 (Ly α) emission extending over $\gtrsim \, \rm 10\, kilo\,parsec\, (kpc)$ around dusty, massive starbursts at z ≳ 3 might represent a short-lived phase in the evolution of present-day, massive quiescent galaxies. To obtain empirical constraints on this emerging scenario, we present Ly α, C ivλ1550 (C iv), and He ii λ1640 (He ii) observations taken with the Multi-Unit Spectroscopic Explorer towards J1000+0234: a galaxy pair at z = 4.5 composed of a low-mass starburst (J1000+0234−South) neighbouring a massive Submillimeter Galaxy (SMG; J1000+0234−North) that harbours a rotationally supported gas disc. Based on the spatial distribution and relative strength of Ly α, C iv, and He ii, we find that star formation in J1000+0234−South and an active galactic nucleus in J1000+0234−North are dominant factors in driving the observed 40 kiloparsec-scale Ly α blob (LAB). We use the non-resonant He ii  line to infer kinematic information of the LAB. We find marginal evidence for two spatially and spectrally separated He ii regions, which suggests that the two-peaked Ly α profile is mainly a result of two overlapping and likely interacting H i clouds. We also report the serendipitous identification of three Ly α emitters spanning over a redshift bin Δz ≤ 0.007 (i.e. $\lesssim 380\, \rm km\, s^{-1}$) located at $\lesssim 140\, \rm kpc$ from J1000+0234. A galaxy overdensity analysis confirms that J1000+0234 lies near the centre of a Megaparsec-scale galaxy overdensity at z = 4.5 that might evolve into a galaxy cluster at z = 0. The properties of J1000+0234 and its large-scale environment strengthen the link between SMGs within LABs, tracing overdense regions, as the progenitors of local massive ellipticals in galaxy clusters.
Keywords (english)
Languageenglish
Publication typeScientific paper - Original scientific paper
Publication statusPublished
Peer reviewPeer review - international
Publication versionPublished version
Journal titleMonthly Notices of the Royal Astronomical Society
Numberingvol. 521, no. 2, pp. 2326-2341
p-ISSN0035-8711
e-ISSN1365-2966
DOIhttps://doi.org/10.1093/mnras/stad594
URN:NBNurn:nbn:hr:217:142972
Publication2023-05
Document URLhttps://academic.oup.com/mnras/article/521/2/2326/7055953
Type of resourceText
Access conditionsOpen access
Terms of useLicence In copyright icon
Public note© 2023 The Author(s). Published by Oxford University Press on behalf of Royal Astronomical Society. Accepted 2023 February 21. Received 2023 February 21; in original form 2022 October 14.
Created on2024-07-22 10:58:50