Parallax Measurements of the Mira-Type Star UX Cygni with Phase-referencing VLBI
- 10 June 2005
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 627 (1), L49-L52
- https://doi.org/10.1086/432051
Abstract
No abstract availableThis publication has 19 references indexed in Scilit:
- Pulsar Parallaxes at 5 GHz with the Very Long Baseline ArrayThe Astrophysical Journal, 2004
- The Vela Pulsar’s Proper Motion and Parallax Derived from VLBI ObservationsThe Astrophysical Journal, 2003
- VLBI astrometry of circumstellar OH masers: Proper motions and parallaxes of four AGB starsAstronomy & Astrophysics, 2003
- An electronic version of the second volume of the General Catalogue of Variable Stars with improved coordinatesAstronomy Letters, 2003
- Reprocessing the Hipparcos data of evolved starsAstronomy & Astrophysics, 2003
- Very Long Baseline Array Measurement of Nine Pulsar ParallaxesThe Astrophysical Journal, 2002
- Extragalactic Radio Source Selection for Use in Directly Linking Optical Astrometric Observations to the Radio Reference FrameThe Astronomical Journal, 2001
- Mira kinematics from Hipparcos data: a Galactic bar to beyond the Solar circleMonthly Notices of the Royal Astronomical Society, 2000
- Mass Loss from Cool Stars: Impact on the Evolution of Stars and Stellar PopulationsAnnual Review of Astronomy and Astrophysics, 2000
- CARBON STARSAnnual Review of Astronomy and Astrophysics, 1998