Zobrazeno 1 - 10
of 44
pro vyhledávání: '"Peter D Mitchell"'
Autor:
Rebecca L. L. Moore, Matthew J. Worrallo, Peter D. Mitchell, Jon Harriman, Katie E. Glen, Robert J. Thomas
Publikováno v:
BMC Biotechnology, Vol 17, Iss 1, Pp 1-11 (2017)
Abstract Background Umbilical cord blood provides a source of hematopoietic stem cells for transplantation with immunological and availability advantages over conventional bone marrow sources. Limited cell numbers and slower engraftment from umbilica
Externí odkaz:
https://doaj.org/article/7ff589392982449aa45159c03eb3ae06
Autor:
Jérémy Blaizot, Thibault Garel, Anne Verhamme, Harley Katz, Taysun Kimm, Léo Michel-Dansac, Peter D Mitchell, Joakim Rosdahl, Maxime Trebitsch
The Ly$\alpha$ line is a powerful probe of distant galaxies, which contains information about inflowing/outflowing gas through which Ly$\alpha$ photons scatter. To develop our understanding of this probe, we post-process a zoom-in radiation-hydrodyna
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c7ebe2f97b58f73919eeddbd447ddc48
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 498(2), 1668-1692
We use the EAGLE suite of hydrodynamical simulations to analyse accretion rates (and the breakdown of their constituent channels) onto haloes over cosmic time, comparing the behaviour of baryons and dark matter (DM). We also investigate the influence
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 504(4), 4817-4828
The physical origin of the scatter in the relation between galaxy stellar mass and the metallicity of the interstellar medium, i.e. the Mass-Metallicity Relation (MZR), reflects the relative importance of key processes in galaxy evolution. The \eagle
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bc47710ccd24478e9edc0a4684702e11
http://hdl.handle.net/1887/3264082
http://hdl.handle.net/1887/3264082
Autor:
Joakim Rosdahl, Peter D. Mitchell, Thibault Garel, Jeremy Blaizot, Yohan Dubois, Corentin Cadiou
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, 2021, 501, pp.5757-5775. ⟨10.1093/mnras/stab035⟩
Monthly Notices of the Royal Astronomical Society, 501(4), 5757-5775
Monthly Notices of the Royal Astronomical Society, 2021, 501, pp.5757-5775. ⟨10.1093/mnras/stab035⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2021, 501, pp.5757-5775. ⟨10.1093/mnras/stab035⟩
Monthly Notices of the Royal Astronomical Society, 501(4), 5757-5775
Monthly Notices of the Royal Astronomical Society, 2021, 501, pp.5757-5775. ⟨10.1093/mnras/stab035⟩
With the Multi Unit Spectroscopic Explorer (MUSE), it is now possible to detect spatially extended Lyman alpha emission from individual faint (M_UV ~ -18) galaxies at redshifts, 3 < z < 6, tracing gas out to circum-galactic scales comparable to the d
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::23eaffa67a428b0f26a962a4a8f2cd2a
http://arxiv.org/abs/2008.12790
http://arxiv.org/abs/2008.12790
Autor:
Camila A. Correa, Claudia del P. Lagos, Peter D. Mitchell, Florencia Collacchioni, Emily Wisnioski, Sofía A. Cora, Joop Schaye
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 495(3), 2827-2843. Oxford University Press
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2020, 495, pp.2827-2843. ⟨10.1093/mnras/staa1334⟩
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Monthly Notices of the Royal Astronomical Society, 495(3), 2827-2843
Collacchioni, F, Lagos, C D P, Mitchell, P D, Schaye, J, Wisnioski, E, Cora, S A & Correa, C A 2020, ' The effect of gas accretion on the radial gas metallicity profile of simulated galaxies ', Monthly Notices of the Royal Astronomical Society, vol. 495, no. 3, pp. 2827-2843 . https://doi.org/10.1093/mnras/staa1334
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2020, 495, pp.2827-2843. ⟨10.1093/mnras/staa1334⟩
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Monthly Notices of the Royal Astronomical Society, 495(3), 2827-2843
Collacchioni, F, Lagos, C D P, Mitchell, P D, Schaye, J, Wisnioski, E, Cora, S A & Correa, C A 2020, ' The effect of gas accretion on the radial gas metallicity profile of simulated galaxies ', Monthly Notices of the Royal Astronomical Society, vol. 495, no. 3, pp. 2827-2843 . https://doi.org/10.1093/mnras/staa1334
We study the effect of the gas accretion rate ($\dot M_{\rm accr}$) on the radial gas metallicity profile (RMP) of galaxies using the EAGLE cosmological hydrodynamic simulations, focusing on central galaxies of stellar mass $M_\star \gtrsim 10^9 \, {
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7551f7fbe77ea530373ff0da1c4bc95d
https://dare.uva.nl/personal/pure/en/publications/the-effect-of-gas-accretion-on-the-radial-gas-metallicity-profile-of-simulated-galaxies(f441613e-e07e-4735-8978-5aa71d60b25e).html
https://dare.uva.nl/personal/pure/en/publications/the-effect-of-gas-accretion-on-the-radial-gas-metallicity-profile-of-simulated-galaxies(f441613e-e07e-4735-8978-5aa71d60b25e).html
Publikováno v:
Monthly Notices of the RAS (0035-8711), 497(4), 4495-4516
Monthly notices of the Royal Astronomical Society, 2020, Vol.497(4), pp.4495-4516 [Peer Reviewed Journal]
Monthly notices of the Royal Astronomical Society, 2020, Vol.497(4), pp.4495-4516 [Peer Reviewed Journal]
The role of galactic wind recycling represents one of the largest unknowns in galaxy evolution, as any contribution of recycling to galaxy growth is largely degenerate with the inflow rates of first-time infalling material, and the rates with which o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::678d68e71529753983d4cb9bc2dab633
http://arxiv.org/abs/2005.10262
http://arxiv.org/abs/2005.10262
Publikováno v:
Monthly Notices of the RAS (0035-8711), 494(3), 3971-3997
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2020, 494, pp.3971-3997. ⟨10.1093/mnras/staa938⟩
Monthly notices of the Royal Astronomical Society, 2020, Vol.484(3), pp.3971-3997 [Peer Reviewed Journal]
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2020, 494, pp.3971-3997. ⟨10.1093/mnras/staa938⟩
Monthly notices of the Royal Astronomical Society, 2020, Vol.484(3), pp.3971-3997 [Peer Reviewed Journal]
We present measurements of galactic outflow rates from the EAGLE suite of cosmological simulations. We find that gas is removed from the interstellar medium (ISM) of central galaxies with a dimensionless mass loading factor that scales approximately
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d5cb18c9482d6c4009269bd7cdae6a51
https://ui.adsabs.harvard.edu/abs/2020MNRAS.494.3971M
https://ui.adsabs.harvard.edu/abs/2020MNRAS.494.3971M
Autor:
Masami Ouchi, Yuma Sugahara, Nicolas Bouché, Yuichi Harikane, Peter D. Mitchell, Jeremy Blaizot
Publikováno v:
The Astrophysical Journal
The Astrophysical Journal, 2019, 886 (1), pp.29. ⟨10.3847/1538-4357/ab49fe⟩
The Astrophysical Journal, American Astronomical Society, 2019, 886 (1), pp.29. ⟨10.3847/1538-4357/ab49fe⟩
Astrophysical Journal (0004-637X), 886(1), 29
The Astrophysical Journal, 2019, 886 (1), pp.29. ⟨10.3847/1538-4357/ab49fe⟩
The Astrophysical Journal, American Astronomical Society, 2019, 886 (1), pp.29. ⟨10.3847/1538-4357/ab49fe⟩
Astrophysical Journal (0004-637X), 886(1), 29
We present velocities of galactic outflows in seven star-forming galaxies at $z=$5-6 with stellar masses of $M_* \sim10^{10.1}\ \rm{M_\odot}$. Although it is challenging to observationally determine the outflow velocities, we overcome this by using A
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ba6ab0300191401b4e21f2945827bf92
https://hdl.handle.net/1887/85016
https://hdl.handle.net/1887/85016
Autor:
Johan Richard, Peter D. Mitchell, Thierry Contini, Johannes Zabl, Ilane Schroetter, Lutz Wisotzki, Sowgat Muzahid, Raffaella Anna Marino, Nicolas Bouché, Martin Wendt, Simon J. Lilly, Joop Schaye, Roland Bacon
Publikováno v:
Monthly Notices of the Royal Astronomical Society: Letters
Monthly Notices of the Royal Astronomical Society: Letters, Oxford Journals, 2019, ⟨10.1093/mnras/stz2822/5586576⟩
Monthly Notices of the Royal Astronomical Society: Letters, 2019, ⟨10.1093/mnras/stz2822/5586576⟩
Monthly Notices of the RAS (0035-8711), 490(3), 4368-4381
Monthly Notices of the Royal Astronomical Society: Letters, Oxford Journals, 2019, ⟨10.1093/mnras/stz2822/5586576⟩
Monthly Notices of the Royal Astronomical Society: Letters, 2019, ⟨10.1093/mnras/stz2822/5586576⟩
Monthly Notices of the RAS (0035-8711), 490(3), 4368-4381
We present results from our on-going MusE GAs FLOw and Wind (MEGAFLOW) survey, which consists of 22 quasar lines-of-sight, each observed with the integral field unit (IFU) MUSE and the UVES spectrograph at the ESO Very Large Telescopes (VLT). The goa
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::920ba8e02d0eb076a1065729ba5d33cc
https://hal.archives-ouvertes.fr/hal-02325516
https://hal.archives-ouvertes.fr/hal-02325516