Pith Number

pith:MPTFI6CH

pith:2026:MPTFI6CHMC4P2ISV6LKNQRGSTO

not attested not anchored not stored refs resolved

BISTRO Survey: Gravity-Dominated and Magnetically Regulated Star Formation in M17 SW

Anthony Whitworth, Archana Soam, Chakali Eswaraiah, Chang Won Lee, David Berry, David Eden, Derek Ward-Thompson, Doris Arzoumanian, Doug Johnstone, Felix Priestley, James Di Francesco, Jihye Hwang, Ji-hyun Kang, Jungmi Kwon, Kate Pattle, Kee-Tae Kim, Keping Qiu, Mengke Zhao, Motohide Tamura, Nguyen Bich Ngoc, Pierre Bastien, Ray S. Furuya, Sarah Sadavoy, Shih-Ping Lai, Takashi Onaka, Thiem Hoang, Tyler L. Bourke, Woojin Kwon, Xindi Tang, Zhiwei Chen

Gravity globally drives star formation in M17 SW while the magnetic field structure regulates it locally.

arxiv:2605.17708 v1 · 2026-05-18 · astro-ph.GA

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Add to your LaTeX paper

\usepackage{pith}
\pithnumber{MPTFI6CHMC4P2ISV6LKNQRGSTO}

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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

✓ Portable graph bundle live · download bundle · merged state

The bundle contains the canonical record plus signed events. A mirror can host it anywhere and recompute the same current state with the deterministic merge algorithm.

Claims

C1strongest claim

Star formation in M17 SW is globally driven by gravity but locally regulated by the magnetic field structure.

C2weakest assumption

The Skalidis-Tassis method applied to the polarization and ammonia data yields accurate plane-of-sky magnetic field strengths without significant residual errors from angle dispersion or unresolved structure (abstract and implied methods section).

C3one line summary

High-resolution magnetic field maps of M17 SW reveal gravity-dominated energy budget with magnetic fields regulating collapse and accretion channels in a near-equipartition state.

References

103 extracted · 103 resolved · 34 Pith anchors

[1] The Astropy Project: Building an inclusive, open-science project and status of the v2.0 core package · doi:10.3847/1538-3881/aabc4f

[2] arXiv , Author =:1307.6212 , Journal = 2013 · doi:10.1051/0004-6361/201322068

[3] 1996, A&AS, 117, 393, doi: 10.1051/aas:1996164 1996 · doi:10.1051/aas:1996164

[4] Quantifying the Observational Effort Required for the Radial Velocity Characterization of TESS Planets 2018 · doi:10.3847/1538-3881/aacea9

[5] X-ray Scattering Echoes and Ghost Halos from the Intergalactic Medium: Relation to the nature of AGN variability 2015 · doi:10.1088/0004-637x/805/1/23

Formal links

2 machine-checked theorem links

Receipt and verification

First computed	2026-05-20T00:04:54.022532Z
Builder	pith-number-builder-2026-05-17-v1
Signature	Pith Ed25519 (`pith-v1-2026-05`) · public key
Schema	pith-number/v1.0

Canonical hash

63e654784760b8fd2255f2d4d844d29ba14c04ea568587090bf1111863796756

Aliases

arxiv: 2605.17708 · arxiv_version: 2605.17708v1 · doi: 10.48550/arxiv.2605.17708 · pith_short_12: MPTFI6CHMC4P · pith_short_16: MPTFI6CHMC4P2ISV · pith_short_8: MPTFI6CH

Agent API

Resolver JSON Graph JSON Events JSON Schema Signing key

Verify this Pith Number yourself

curl -sH 'Accept: application/ld+json' https://pith.science/pith/MPTFI6CHMC4P2ISV6LKNQRGSTO \
  | 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: 63e654784760b8fd2255f2d4d844d29ba14c04ea568587090bf1111863796756

Canonical record JSON

{
  "metadata": {
    "abstract_canon_sha256": "3875dad3bae6b3f9f15a848f341765da0b1b9797dd533b1787586de415dfdc8a",
    "cross_cats_sorted": [],
    "license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
    "primary_cat": "astro-ph.GA",
    "submitted_at": "2026-05-18T00:07:32Z",
    "title_canon_sha256": "57f9d44cab68c548bc6cf0212d4a5d1813d419090c21d4b50bd62025426d813a"
  },
  "schema_version": "1.0",
  "source": {
    "id": "2605.17708",
    "kind": "arxiv",
    "version": 1
  }
}