Hostname: page-component-84b7d79bbc-tsvsl Total loading time: 0 Render date: 2024-07-25T07:38:53.268Z Has data issue: false hasContentIssue false
  • English
  • Français

7.17. A possibility of measurement of distance and proper motion of galactic sources by using a differential VLBI method of VERA

Published online by Cambridge University Press:  25 May 2016

O. Kameya ,
T. Sasao  and
M. Miyoshi
O. Kameya
Affiliation:
National Astronomical Observatory, Mizusawa 2-12 Hoshigaoka, Mizusawa, Iwate 023, Japan kameya@miz.nao.ac.jp
T. Sasao
Affiliation:
National Astronomical Observatory, Mizusawa 2-12 Hoshigaoka, Mizusawa, Iwate 023, Japan sasao@miz.nao.ac.jp
M. Miyoshi
Affiliation:
National Astronomical Observatory, Mizusawa 2-12 Hoshigaoka, Mizusawa, Iwate 023, Japan miyoshi@miz.nao.ac.jp

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

National Astronomical Observatory, Japan has a plan to construct a new VLBI system named VERA (VLBI Exploration of Radio Astrometry). The system can measure precise positions of Galactic radio sources (H2O masers and SiO masers) referring to adjacent radio sources (QSO etc.) by using a differential VLBI method (Sasao and Morimoto, 1991).

Type
Part II. Nuclear Interstellar Medium
Information
Symposium - International Astronomical Union , Volume 184: The Central Regions of the Galaxy and Galaxies , 1998 , pp. 327 - 328
Copyright
Copyright © Kluwer 1998 

References

Alberdi, A., Lara, L., Marcaido, J.M., Elosegui, P., Shapiro, I.I., Cotton, W.D., Diamond, P.J., Romney, J.D., and Preston, R.A. (1993), VLBI image of SgrA* at λ=1.35 cm, Astron. Astrophy., 277, pp.L1–L4.Google Scholar
Sasao, T., and Moriomoto, M. (1991), Antennacluster-antennacluster VLBI for geodesy and astrometry, in Chapmann Conference on Geodetic VLBI: Monitoring Global Change, NOAA, Tech. Rep. NOS 137 NGS49, pp.48–62.Google Scholar