Interstellar scintillation is an indicator of astrometric stability
arXiv:1306.4398 · doi:10.1093/mnras/stt1049
Abstract
We examine the relationship between astrometric stability and astrophysical properties in flat-spectrum radio-loud quasars making up the celestial reference frame. We use position determinations from geodetic VLBI measurements, and develop a new metric for source position stability. We then compare this quantity to two measures of source compactness: structure index, which probes structure on milliarcsecond scales; and the presence of interstellar scintillation associated with the quasar, which probes scales of tens of microarcseconds. We find that persistent scintillators have greater position stability than episodic scintillators, which are in turn more stable than non-scintillators. Scintillators are also more likely to be compact on milliarcsecond scales, as measured by the structure index. Persistent scintillators are therefore excellent candidates for inclusion in any future realisation of the celestial reference frame. A list of these sources is presented in the Appendix. We find that slow (characteristic timescale >3 days) scintillators have more stable positions than rapid scintillators, suggesting they are more compact. High-cadence, long term monitoring is therefore required to identify other members of this population of compact, high brightness temperature quasars.
11 pages, 12 figures, 1 table. Accepted for publication in MNRAS
References in corpus (6)
- Trigonometric Parallaxes of Massive Star Forming Regions: VI. Galactic Structure, Fundamental Parameters and Non-Circular Motions
- The Micro-Arcsecond Scintillation-Induced Variability (MASIV) Survey II: The First Four Epochs
- Galaxy Zoo: dust lane early-type galaxies are tracers of recent, gas-rich minor mergers
- The AuScope Geodetic VLBI Array
- First Stellar Velocity Dispersion Measurement of a Luminous Quasar Host with Gemini North Laser Guide Star Adaptive Optics
- BL LAC PKSB1144-379 an extreme scintillator