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pith:PF7ZPJ7B

pith:2019:PF7ZPJ7BOQAYGJLJVWT7OXCRXH
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First Results from the TNG50 Simulation: Galactic outflows driven by supernovae and black hole feedback

Annalisa Pillepich, Dylan Nelson, Federico Marinacci, Lars Hernquist, Mark Vogelsberger, Paul Torrey, Rainer Weinberger, Ruediger Pakmor, Shy Genel, Volker Springel

In this high-resolution cosmological simulation, galactic outflow mass loading turns non-monotonic with stellar mass and rises rapidly above 10^10.5 solar masses due to central black hole feedback.

arxiv:1902.05554 v2 · 2019-02-14 · astro-ph.GA · astro-ph.CO · astro-ph.HE

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\pithnumber{PF7ZPJ7BOQAYGJLJVWT7OXCRXH}

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Record completeness

1 Bitcoin timestamp
2 Internet Archive
3 Author claim open · sign in to claim
4 Citations open
5 Replications open
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Claims

C1strongest claim

Outflow mass loading is a non-monotonic function of galaxy stellar mass, turning over and rising rapidly above 10^10.5 Msun due to the action of the central black hole.

C2weakest assumption

The subgrid prescriptions for supernova and black hole feedback, including their energy injection and wind scalings, are assumed to produce realistic large-scale outflows when the simulation resolution reaches ~100 pc.

C3one line summary

TNG50 shows galactic outflow mass loading is non-monotonic with stellar mass, rising rapidly above 10^10.5 Msun due to black hole feedback, and produces fast multi-phase outflows with emergent collimation.

References

300 extracted · 300 resolved · 14 Pith anchors

[1] Simulations of Galaxy Formation in a Cold Dark Matter Universe. I. Dynamical and Photometric Properties of a Simulated Disk Galaxy. , eprint =. doi:10.1086/375512 , adsurl = · doi:10.1086/375512
[2] M., & Spurzem, R 2007 · doi:10.1111/j.1365-2966.2007.12183.x
[3] 2009, MNRAS, 395, L6, doi: 10.1111/j.1745-3933.2009.00627.x 2009 · doi:10.1111/j.1745-3933.2009.00685.x
[4] , archivePrefix = "arXiv", eprint = · doi:10.1088/0004-637x/770/1/25
[5] ArXiv e-prints , archivePrefix = "arXiv", eprint =

Formal links

1 machine-checked theorem link

Cited by

26 papers in Pith

Receipt and verification
First computed 2026-05-17T23:38:48.109512Z
Builder pith-number-builder-2026-05-17-v1
Signature Pith Ed25519 (pith-v1-2026-05) · public key
Schema pith-number/v1.0

Canonical hash

797f97a7e17401832569ada7f75c51b9c7577dfc5e8916b239c3293806cfe2e4

Aliases

arxiv: 1902.05554 · arxiv_version: 1902.05554v2 · doi: 10.48550/arxiv.1902.05554 · pith_short_12: PF7ZPJ7BOQAY · pith_short_16: PF7ZPJ7BOQAYGJLJ · pith_short_8: PF7ZPJ7B
Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/PF7ZPJ7BOQAYGJLJVWT7OXCRXH \
  | jq -c '.canonical_record' \
  | python3 -c "import sys,json,hashlib; b=json.dumps(json.loads(sys.stdin.read()), sort_keys=True, separators=(',',':'), ensure_ascii=False).encode(); print(hashlib.sha256(b).hexdigest())"
# expect: 797f97a7e17401832569ada7f75c51b9c7577dfc5e8916b239c3293806cfe2e4
Canonical record JSON
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      "astro-ph.CO",
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    ],
    "license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
    "primary_cat": "astro-ph.GA",
    "submitted_at": "2019-02-14T19:00:00Z",
    "title_canon_sha256": "467e7c3638be930f59d55738bfd4f3fd4b6a7b58817010983c773d0e95c93c70"
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}