Paper Citation Record · LEDGER

Modeling Nonaxisymmetric Bow Shocks: Solution Method and Exact Analytic Solutions

As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:astro-ph/0003389.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
astro-ph/0003389 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-14T06:32:32.682623+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T20:40:57.067610Z

measured 1 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: pith, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
unresolved0
parse uncertain0
malformed identifier0
metadata mismatch0

External citation measurements

80
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 91927d80-d696-4034-941e-c6122d55d300 · inbound

Guitar Nebula: extreme accelerator in extreme environment cites this paper.

Guitar Nebula: extreme accelerator in extreme environment Modeling Nonaxisymmetric Bow Shocks: Solution Method and Exact Analytic Solutions

Reference 69

Resolution: verified exact; local_arxiv, observed 2026-05-14T17:52:31.627076Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation a3d27d4b-4b8d-442e-946c-07e3916e4823 · inbound

An Halpha survey of infrared bow-shocks around OB-type stars cites this paper.

An Halpha survey of infrared bow-shocks around OB-type stars Modeling Nonaxisymmetric Bow Shocks: Solution Method and Exact Analytic Solutions

Reference 48

Resolution: unresolved; no resolver link, observed 2026-07-31T12:04:43.216272Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation dea0047d-c318-4f4d-b6fb-f2ddca927871 · inbound

Why do massive stars form bow shocks? Bulk ISM motion as the main driver of bow shock formation and geometry cites this paper.

Why do massive stars form bow shocks? Bulk ISM motion as the main driver of bow shock formation and geometry Modeling Nonaxisymmetric Bow Shocks: Solution Method and Exact Analytic Solutions

Reference 66

Resolution: unresolved; no resolver link, observed 2026-08-07T20:40:57.067610Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.