Indications of an Unmodelled Component in Spectrographic Measurements of Local Stars
Charles Francis, Erik Anderson

TL;DR
This study suggests that an unmodelled component in spectrographic measurements of stellar radial velocities may explain the observed flat rotation curves of galaxies, challenging dark matter and modified gravity theories.
Contribution
It provides evidence for an unmodelled spectrographic component affecting radial velocity measurements, offering an alternative explanation for galaxy rotation curves.
Findings
Statistical test rejects systematic errors in radial velocity measurements.
Tension observed in orbital velocity calculations from different star populations.
Proposes a cosmological origin for the unmodelled component affecting measurements.
Abstract
Context: While CDM models and MOND give explanations for flat rotation curves of other galaxies, both present observational problems and the local gradient of the Milky Way's rotation curve is not flat. Aims: We consider whether flat rotation curves could be an artifact of an unmodelled component in spectral shift. Methods: In the absence of astrometric determinations of radial velocity, we apply a statistical test on a population of 20 440 Hipparcos stars inside 300 pc with known radial velocities and with accurate parallaxes in the New Hipparcos Reduction. Results: The test rejects the null hypothesis, there is no systematic error in spectrographic determinations of heliocentric radial velocity, with 99.95% confidence. In a separate test on metal-poor stars, we find tension between calculations of the orbital velocity of the Sun from three populations of halo stars inside and outside…
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Taxonomy
TopicsAstronomy and Astrophysical Research · Statistical and numerical algorithms · Scientific Research and Discoveries
