Bipolar outflows out to 10 kpc for massive galaxies at redshift z ≈ 1.


Journal

Nature
ISSN: 1476-4687
Titre abrégé: Nature
Pays: England
ID NLM: 0410462

Informations de publication

Date de publication:
Dec 2023
Historique:
received: 22 02 2023
accepted: 04 10 2023
medline: 11 12 2023
pubmed: 7 12 2023
entrez: 6 12 2023
Statut: ppublish

Résumé

Galactic outflows are believed to play a critical role in the evolution of galaxies by regulating their mass build-up and star formation

Identifiants

pubmed: 38057569
doi: 10.1038/s41586-023-06718-w
pii: 10.1038/s41586-023-06718-w
doi:

Types de publication

Journal Article

Langues

eng

Sous-ensembles de citation

IM

Pagination

53-56

Informations de copyright

© 2023. The Author(s), under exclusive licence to Springer Nature Limited.

Références

Tumlinson, J., Peeples, M. S. & Werk, J. K. The circumgalactic medium. Annu. Rev. Astron. Astrophys. 55, 389–432 (2017).
doi: 10.1146/annurev-astro-091916-055240
Predehl, P. et al. Detection of large-scale X-ray bubbles in the Milky Way halo. Nature 588, 227–231 (2020).
pubmed: 33299190 doi: 10.1038/s41586-020-2979-0
Bland, J. & Tully, B. Large-scale bipolar wind in M82. Nature 334, 43–45 (1988).
doi: 10.1038/334043a0
Muratov, A. L. et al. Gusty, gaseous flows of FIRE: galactic winds in cosmological simulations with explicit stellar feedback. Mon. Not. R. Astron. Soc. 454, 2691–2713 (2015).
doi: 10.1093/mnras/stv2126
Bacon, R. et al. The MUSE second-generation VLT instrument. Proc. SPIE 7735, 773508 (2010).
doi: 10.1117/12.856027
Morrissey, P. et al. The Keck Cosmic Web Imager integral field spectrograph. Astrophys. J. 864, 93 (2018).
doi: 10.3847/1538-4357/aad597
Wisotzki, L. et al. Extended Lyman α haloes around individual high-redshift galaxies revealed by MUSE. Astron. Astrophys. 587, A98 (2016).
doi: 10.1051/0004-6361/201527384
Wisotzki, L. et al. Nearly all the sky is covered by Lyman-α emission around high-redshift galaxies. Nature 562, 229–232 (2018).
pubmed: 30275476 doi: 10.1038/s41586-018-0564-6
Leclercq, F. et al. The MUSE Hubble Ultra Deep Field Survey. VIII. Extended Lyman-α haloes around high-z star-forming galaxies. Astron. Astrophys. 608, A8 (2017).
doi: 10.1051/0004-6361/201731480
Cai, Z. et al. Evolution of the cool gas in the circumgalactic medium of massive halos: a Keck Cosmic Web Imager survey of Lyα emission around QSOs at z ≈ 2. Astrophys. J. Suppl. Ser. 245, 23 (2019).
doi: 10.3847/1538-4365/ab4796
Kusakabe, H. et al. The MUSE eXtremely Deep Field: individual detections of Lyα haloes around rest-frame UV-selected galaxies at z ≃ 2.9–4.4. Astron. Astrophys. 660, A44 (2022).
doi: 10.1051/0004-6361/202142302
Bacon, R. et al. The MUSE Extremely Deep Field: the cosmic web in emission at high redshift. Astron. Astrophys. 647, A107 (2021).
doi: 10.1051/0004-6361/202039887
Guo, Y. et al. Metal enrichment in the circumgalactic medium and Lyα halos around quasars at z ~ 3. Astrophys. J. 898, 26 (2020).
doi: 10.3847/1538-4357/ab9b7f
Johnson, S. D. et al. Directly tracing cool filamentary accretion over >100 kpc into the interstellar medium of a quasar host at z = 1. Astrophys. J. Lett. 940, L40 (2022).
doi: 10.3847/2041-8213/aca28e
Herenz, E. C. et al. A ~15 kpc outflow cone piercing through the halo of the blue compact metal-poor galaxy SBS0335–052E. Astron. Astrophys. 670, A121 (2023).
doi: 10.1051/0004-6361/202244930
Kacprzak, G. G., Cooke, J., Churchill, C. W., Ryan-Weber, E. V. & Nielsen, N. M. The smooth Mg II gas distribution through the interstellar/extra-planar/halo interface. Astrophys. J. Lett. 777, L11 (2013).
doi: 10.1088/2041-8205/777/1/L11
Rubin, K. H. R. et al. Low-ionization line emission from a starburst galaxy: a new probe of a galactic-scale outflow. Astrophys. J. 728, 55 (2011).
doi: 10.1088/0004-637X/728/1/55
Martin, C. L. et al. Scattered emission from z ~ 1 galactic outflows. Astrophys. J. 770, 41 (2013).
doi: 10.1088/0004-637X/770/1/41
Burchett, J. N. et al. Circumgalactic Mg II emission from an isotropic starburst galaxy outflow mapped by KCWI. Astrophys. J. 909, 151 (2021).
doi: 10.3847/1538-4357/abd4e0
Zabl, J. et al. MusE GAs FLOw and Wind (MEGAFLOW) VIII. Discovery of a MgII emission halo probed by a quasar sightline. Mon. Not. R. Astron. Soc. 507, 4294–4315 (2021).
doi: 10.1093/mnras/stab2165
Leclercq, F. et al. The MUSE eXtremely deep field: first panoramic view of an Mg II emitting intragroup medium. Astron. Astrophys. 663, A11 (2022).
doi: 10.1051/0004-6361/202142179
Bacon, R. et al. The MUSE Hubble Ultra Deep Field surveys: data release II. Astron. Astrophys. 670, A4 (2023).
doi: 10.1051/0004-6361/202244187
Kornei, K. A. et al. The properties and prevalence of galactic outflows at z ~ 1 in the Extended Groth Strip. Astrophys. J. 758, 135 (2012).
doi: 10.1088/0004-637X/758/2/135
Feltre, A. et al. The MUSE Hubble Ultra Deep Field Survey. XII. Mg II emission and absorption in star-forming galaxies. Astron. Astrophys. 617, A62 (2018).
doi: 10.1051/0004-6361/201833281
Bouché, N. et al. Physical properties of galactic winds using background quasars. Mon. Not. R. Astron. Soc. 426, 801–815 (2012).
doi: 10.1111/j.1365-2966.2012.21114.x
Zabl, J. et al. MusE GAs FLOw and Wind (MEGAFLOW) II. A study of gas accretion around z ≈ 1 star-forming galaxies with background quasars. Mon. Not. R. Astron. Soc. 485, 1961–1980 (2019).
doi: 10.1093/mnras/stz392
Martin, C. L., Ho, S. H., Kacprzak, G. G. & Churchill, C. W. Kinematics of circumgalactic gas: feeding galaxies and feedback. Astrophys. J. 878, 84 (2019).
doi: 10.3847/1538-4357/ab18ac
Schroetter, I. et al. MusE GAs FLOw and Wind (MEGAFLOW) – III. Galactic wind properties using background quasars. Mon. Not. R. Astron. Soc. 490, 4368–4381 (2019).
doi: 10.1093/mnras/stz2822
Muratov, A. L. et al. Metal flows of the circumgalactic medium, and the metal budget in galactic haloes. Mon. Not. R. Astron. Soc. 468, 4170–4188 (2017).
doi: 10.1093/mnras/stx667
Péroux, C. et al. Predictions for the angular dependence of gas mass flow rate and metallicity in the circumgalactic medium. Mon. Not. R. Astron. Soc. 499, 2462–2473 (2020).
doi: 10.1093/mnras/staa2888
Claeyssens, A. et al. Spectral variations of Lyman α emission within strongly lensed sources observed with MUSE. Mon. Not. R. Astron. Soc. 489, 5022–5029 (2019).
doi: 10.1093/mnras/stz2492
Leclercq, F. et al. The MUSE Hubble Ultra Deep Field Survey. XIII. Spatially resolved spectral properties of Lyman α haloes around star-forming galaxies at z > 3. Astron. Astrophys. 635, A82 (2020).
doi: 10.1051/0004-6361/201937339
Erb, D. K. et al. The circumgalactic medium of extreme emission line galaxies at z~2: resolved spectroscopy and radiative transfer modeling of spatially extended Lyα emission in the KBSS-KCWI survey. Astrophys. J. 953, 118 (2023).
doi: 10.3847/1538-4357/acd849
Bacon, R. et al. The MUSE Hubble Ultra Deep Field Survey. I. Survey description, data reduction, and source detection. Astron. Astrophys. 608, A1 (2017).
doi: 10.1051/0004-6361/201730833
Bouché, N. F. et al. The MUSE Hubble Ultra Deep Field Survey. XVI. The angular momentum of low-mass star-forming galaxies: A cautionary tale and insights from TNG50. Astron. Astrophys. 654, A49 (2021).
doi: 10.1051/0004-6361/202040225
Rubin, K. H. R. et al. Evidence for ubiquitous collimated galactic-scale outflows along the star-forming sequence at z ~ 0.5. Astrophys. J. 794, 156 (2014).
doi: 10.1088/0004-637X/794/2/156
Walter, F., Weiss, A. & Scoville, N. Molecular gas in M82: resolving the outflow and streamers. Astrophys. J. 580, L21 (2002).
doi: 10.1086/345287
Chisholm, J., Prochaska, J. X., Schaerer, D., Gazagnes, S. & Henry, A. Optically thin spatially resolved Mg II emission maps the escape of ionizing photons. Mon. Not. R. Astron. Soc. 498, 2554–2574 (2020).
doi: 10.1093/mnras/staa2470
Katz, H. et al. Mg II in the JWST era: a probe of Lyman continuum escape?. Mon. Not. R. Astron. Soc. 515, 4265–4286 (2022).
doi: 10.1093/mnras/stac1437
Bordoloi, R. et al. The radial and azimuthal profiles of Mg II absorption around 0.5 < z < 0.9 zCOSMOS galaxies of different colors, masses, and environments. Astrophys. J. 743, 10 (2011).
doi: 10.1088/0004-637X/743/1/10
Kacprzak, G. G., Churchill, C. W. & Nielsen, N. M. Tracing outflows and accretion: a bimodal azimuthal dependence of Mg II absorption. Astrophys. J. Lett. 760, L7 (2012).
doi: 10.1088/2041-8205/760/1/L7
Bordoloi, R., Lilly, S. J., Kacprzak, G. G. & Churchill, C. W. Modeling the distribution of Mg II absorbers around galaxies using background galaxies and quasars. Astrophys. J. 784, 108 (2014).
doi: 10.1088/0004-637X/784/2/108
Lan, T.-W. & Mo, H. The circumgalactic medium of eBOSS emission line galaxies: signatures of galactic outflows in gas distribution and kinematics. Astrophys. J. 866, 36 (2018).
doi: 10.3847/1538-4357/aadc08
Lundgren, B. F. et al. The geometry of cold, metal-enriched gas around galaxies at z ~ 1.2. Astrophys. J. 913, 50 (2021).
doi: 10.3847/1538-4357/abef6a
Chen, Y.-M. et al. Absorption-line probes of the prevalence and properties of outflows in present-day star-forming galaxies. Astrophys. J. 140, 445 (2010).
Bordoloi, R. et al. The dependence of galactic outflows on the properties and orientation of zCOSMOS galaxies at z ~ 1. Astrophys. J. 794, 130 (2014).
doi: 10.1088/0004-637X/794/2/130
Shaban, A. et al. A 30 kpc spatially extended clumpy and asymmetric galactic outflow at z ~ 1.7. Astrophys. J. 936, 77 (2022).
doi: 10.3847/1538-4357/ac7c65
Rupke, D. S. N. et al. A 100-kiloparsec wind feeding the circumgalactic medium of a massive compact galaxy. Nature 574, 643–646 (2019).
pubmed: 31666723 doi: 10.1038/s41586-019-1686-1
Sobolev, V. V. Moving Envelopes of Stars (Harvard University Press, 1960) [transl.].
Carr, C., Scarlata, C., Panagia, N. & Henry, A. A Semi-analytical Line Transfer (SALT) Model. II: the effects of a bi-conical geometry. Astrophys. J. 860, 143 (2018).
doi: 10.3847/1538-4357/aac48e
Zahid, H. J., Kewley, L. J. & Bresolin, F. The mass–metallicity and luminosity–metallicity relations from DEEP2 at z ~ 0.8. Astrophys. J. 730, 137 (2011).
doi: 10.1088/0004-637X/730/2/137
Kennicutt, R. C. Star formation in galaxies along the Hubble sequence. Annu. Rev. Astron. Astrophys. 36, 189–231 (1998).
doi: 10.1146/annurev.astro.36.1.189
Mitchell, P. D. & Schaye, J. How gas flows shape the stellar–halo mass relation in the EAGLE simulation. Mon. Not. R. Astron. Soc. 511, 2948–2967 (2022).
doi: 10.1093/mnras/stab3339

Auteurs

Yucheng Guo (Y)

Univ Lyon, Univ Lyon1, Ens de Lyon, CNRS, Centre de Recherche Astrophysique de Lyon UMR5574, Saint-Genis-Laval, France. yucheng.guo@univ-lyon1.fr.

Roland Bacon (R)

Univ Lyon, Univ Lyon1, Ens de Lyon, CNRS, Centre de Recherche Astrophysique de Lyon UMR5574, Saint-Genis-Laval, France.

Nicolas F Bouché (NF)

Univ Lyon, Univ Lyon1, Ens de Lyon, CNRS, Centre de Recherche Astrophysique de Lyon UMR5574, Saint-Genis-Laval, France.

Lutz Wisotzki (L)

Leibniz-Institut für Astrophysik Potsdam (AIP), Potsdam, Germany.

Joop Schaye (J)

Leiden Observatory, Leiden University, Leiden, The Netherlands.

Jérémy Blaizot (J)

Univ Lyon, Univ Lyon1, Ens de Lyon, CNRS, Centre de Recherche Astrophysique de Lyon UMR5574, Saint-Genis-Laval, France.

Anne Verhamme (A)

Observatoire de Genève, Université de Genève, Versoix, Switzerland.

Sebastiano Cantalupo (S)

Dipartimento di Fisica "G. Occhialini", Università degli Studi di Milano Bicocca, Milano, Italy.

Leindert A Boogaard (LA)

Max Planck Institute for Astronomy, Heidelberg, Germany.

Jarle Brinchmann (J)

Leiden Observatory, Leiden University, Leiden, The Netherlands.
Instituto de Astrofísica e Ciências do Espaço, Centro de Astrofísica da Universidade do Porto (CAUP), Porto, Portugal.

Maxime Cherrey (M)

Univ Lyon, Univ Lyon1, Ens de Lyon, CNRS, Centre de Recherche Astrophysique de Lyon UMR5574, Saint-Genis-Laval, France.

Haruka Kusakabe (H)

Observatoire de Genève, Université de Genève, Versoix, Switzerland.
National Astronomical Observatory of Japan (NAOJ), Mitaka, Tokyo, Japan.

Ivanna Langan (I)

Univ Lyon, Univ Lyon1, Ens de Lyon, CNRS, Centre de Recherche Astrophysique de Lyon UMR5574, Saint-Genis-Laval, France.
European Southern Observatory, Garching, Germany.

Floriane Leclercq (F)

Department of Astronomy, The University of Texas at Austin, Austin, TX, USA.

Jorryt Matthee (J)

Department of Physics, ETH Zürich, Zürich, Switzerland.

Léo Michel-Dansac (L)

Univ Lyon, Univ Lyon1, Ens de Lyon, CNRS, Centre de Recherche Astrophysique de Lyon UMR5574, Saint-Genis-Laval, France.

Ilane Schroetter (I)

Institut de Recherche en Astrophysique et Planétologie, Université Toulouse III - Paul Sabatier, CNRS, CNES, Toulouse Cedex 04, France.

Martin Wendt (M)

Institut für Physik und Astronomie, Universität Potsdam, Golm, Germany.

Classifications MeSH