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Spatially resolved spectroscopic analysis of Ly¿ haloes

Title
Spatially resolved spectroscopic analysis of Ly¿ haloes
Type
Article in International Scientific Journal
Year
2024
Authors
Guo, YC
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Bacon, R
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Wisotzki, L
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Garel, T
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Blaizot, J
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Schaye, J
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Matthee, J
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Leclercq, F
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Boogaard, L
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Richard, J
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Verhamme, A
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J. Brinchmann
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Michel-Dansac, L
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Kusakabe, H
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Journal
Vol. 691
Final page: A66
ISSN: 0004-6361
Publisher: EDP Sciences
Other information
Authenticus ID: P-017-G4E
Abstract (EN): The extended Ly alpha haloes (LAHs) have been found to be prevalent around high-redshift star-forming galaxies. However, the origin of the LAHs is still a subject of debate. The spatially resolved analysis of Ly alpha profiles provides an important diagnostic. We analyse the average spatial extent and spectral variation of the circumgalactic LAHs by stacking a sample of 155 Ly alpha emitters (LAEs) at redshifts of 3 < z < 4 in the MUSE Extremely Deep Field. Our analysis reveals that, with respect to the Ly alpha line of the target LAE, the peak of the Ly alpha line at large distances becomes increasingly more blueshifted up to a projected distance of 60 kpc (approximate to 3x virial radius), with a velocity offset of approximate to 250 km/s. This trend is evident in both the mean and median stacks, suggesting that it is a general property of our LAE sample, which typically has a Ly alpha luminosity of approximate to 10(41.1) erg s(-1). However, due to the absence of systemic redshift data, it remains unclear whether the Ly alpha line peak at large projected distances is less redshifted compared to the inner regions or truly blueshifted with respect to the systemic velocity. We explore various scenarios to explain the large-scale kinematics of the Ly alpha line.
Language: English
Type (Professor's evaluation): Scientific
No. of pages: 9
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