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The outer halo globular cluster system of M31 - III. Relationship to the stellar halo

Autor: P. Cote, Annette M. N. Ferguson, Nicolas F. Martin, Alan W. McConnachie, Geraint F. Lewis, Nial R. Tanvir, Nicholas F. Bate, Rodrigo A. Ibata, Michelle L. M. Collins, Mike Irwin, Alasdair Mackey, Avon Huxor, Jovan Veljanoski

Publikováno v: Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2019, 484 (2), pp.1756-1789. ⟨10.1093/mnras/stz072⟩
Monthly Notices of the Royal Astronomical Society, 484(2), 1756-1789. Oxford University Press
Mackey, D, Ferguson, A, Huxor, A, Veljanoski, J, Lewis, G, McConnachie, A, Ibata, R, Irwin, M, Côté, P, Collins, M, Tanvir, N & Bate, N 2019, ' The outer halo globular cluster system of M31-III. Relationship to the stellar halo ', Monthly Notices of the Royal Astronomical Society, vol. 484, no. 2, pp. 1756–1789 . https://doi.org/10.1093/mnras/stz072
Mackey, D, Ferguson, A, Huxor, A, Veljanoski, J, Lewis, G, McConnachie, A, Martin, N, Ibata, R, Irwin, M, Côté, P, Collins, M, Tanvir, N & Bate, N 2019, ' Outer halo globular cluster system of M31-III. Relationship to the stellar halo ', Monthly Notices of the Royal Astronomical Society, vol. 484, no. 2, pp. 1756–1789 . https://doi.org/10.1093/mnras/stz072

We utilise the final catalogue from the Pan-Andromeda Archaeological Survey to investigate the links between the globular cluster system and field halo in M31 at projected radii $R_p=25-150$ kpc. In this region the cluster radial density profile exhi

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4bd0984f8b42de576e4df076ae413654
https://www.repository.cam.ac.uk/handle/1810/291994

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Detection of warm and cold phases of the neutral ISM in a damped Ly alpha absorber

Publikováno v: The Astrophysical Journal. 532(1):146-151

present a detailed study of the HI 21 cm absorption system at z = 0.0912 toward the radio quasar B0738+313. The uncommonly narrow main absorption line and weak secondary line are resolved for the first time and have FWHM velocities of Delta v(1) = 3.

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=dris___01423::93f1cf485b222ab9cba2378a019f63d3
https://research.rug.nl/en/publications/59b7f7f6-792f-441b-a489-ea228b8ff014

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