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Sökning: WFRF:(Nakagawa H) > Konferensbidrag

  • Resultat 1-10 av 17
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  • Tanaka, Y. K., et al. (författare)
  • WASA-FRS EXPERIMENTS IN FAIR PHASE-0 AT GSI
  • 2023
  • Ingår i: ACTA PHYSICA POLONICA B PROCEEDINGS SUPPLEMENT. - : Jagiellonian University.
  • Konferensbidrag (refereegranskat)abstract
    • We have developed a new and unique experimental setup integrating the central part of the Wide Angle Shower Apparatus (WASA) into the Fragment Separator (FRS) at GSI. This combination opens up possibilities of new experiments with high-resolution spectroscopy at forward 0 and measurements of light decay particles with nearly full solid-angle acceptance in coincidence. The first series of the WASA-FRS experiments have been successfully carried out in 2022. The developed experimental setup and two physics experiments performed in 2022 including the status of the preliminary data analysis are introduced.
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  • Larsen, H-C, et al. (författare)
  • Age- and sex-related postural change
  • 2000
  • Ingår i: Equilibrium research, clinical equilibriometry and modern treatment. - Amsterdam : Elsevier. - 044450012X - 9780444500120 ; , s. 293-293
  • Konferensbidrag (refereegranskat)
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  • van Langevelde, H. J., et al. (författare)
  • The Synergy between VLBI and Gaia astrometry
  • 2018
  • Ingår i: Proceedings of Science. - 1824-8039. ; 344
  • Konferensbidrag (refereegranskat)abstract
    • With the publication of Gaia DR2, 1.3 billion stars now have public parallax and proper motion measurements. In this contribution, we compare the results for sources that have both optical and radio measurements, focusing on circumstellar masers. For these large, variable and bright AGB stars, the VLBI astrometry results can be more robust. Moreover, there are a number of applications where VLBI astrometry provides unique data for studying stellar populations and Galactic structure. The BeSSel project not only provides parallax and proper motions at much larger distances than Gaia can reach, but it also uniquely samples the spiral arms of the Galaxy. The evolved stars in the BAaDE sample can potentially constrain the dynamics and stellar content of the inner bulge and bar of the Milky Way, not reachable in the optical.
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  • Resultat 1-10 av 17

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