Skip to content
DraconiticResearch
Search Sources API
194,220 studies31 sourcesUpdated 15 min ago
PreprintCC BY 4.0arXiv

Stellar proper motions compared with the plane-of-sky magnetic field

Abstract

6 pages, 1 figure, 2 tables. Separates the motions superposed in a young star's proper motion, solar reflex, Galactic rotation, the cloud's own space velocity, subgroup motion and internal flow, and asks which of them a field-alignment statistic actually measures. v4: adds a frame-independent bound on the alignment amplitude; adds an independent check of the bulk motion left by the LSR frame against Kounkel et al. (2022) for Orion A North; corrects one reference; journal-neutral formatting.

Related

  1. HURACAN: A comparison of stellar and interstellar proper motions inside L1688
    M. Piecka, J. Alves, A. Rottensteiner +3
    arXivPreprintCC BY 4.0Full textGalaxiesarXiv
  2. A posteriori correction of Gaia CRF proper motions using conditional probability and zero-parallax prior
    Valeri V. Makarov
    arXivPreprintarXiv licenceFull textGalaxiesarXiv
  3. Kinematic Map of the Galactic Bulge Using HST Proper Motions
    Zhenhao Wang, Shude Mao, Hongjing Yang +3
    arXivPreprintCC BY 4.0Full textGalaxiesarXiv
  4. Observing the Peculiar Acceleration of our Solar System with Quasar Proper Motions
    Phu Huy Nguyen, Calum Murray
    arXivPreprintarXiv licenceFull textCosmologyGalaxiesarXiv
  5. GetGaia 2.0: automatic membership and systemic motions of stellar systems with Gaia
    Andrés del Pino
    arXivPreprintarXiv licenceFull textGalaxiesInstrumentation & methodsarXiv
BibTeX
@misc{ansari2026stellar,
  title = {{Stellar proper motions compared with the plane-of-sky magnetic field}},
  author = {S. G. Ansari},
  howpublished = {arXiv},
  year = {2026},
  month = sep,
  doi = {10.48550/arxiv.2606.19094},
  eprint = {2606.19094},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2606.19094},
  note = {CC BY 4.0},
}
RIS
TY  - UNPB
TI  - Stellar proper motions compared with the plane-of-sky magnetic field
AU  - S. G. Ansari
PY  - 2026
DA  - 2026/09/04
PB  - arXiv
DO  - 10.48550/arxiv.2606.19094
UR  - https://arxiv.org/abs/2606.19094
AB  - 6 pages, 1 figure, 2 tables. Separates the motions superposed in a young star's proper motion, solar reflex, Galactic rotation, the cloud's own space velocity, subgroup motion and internal flow, and asks which of them a field-alignment statistic actually measures. v4: adds a frame-independent bound on the alignment amplitude; adds an independent check of the bulk motion left by the LSR frame against Kounkel et al. (2022) for Orion A North; corrects one reference; journal-neutral formatting.
ER  -