SiO MASERS IN ASYMMETRIC MIRAS. II. R CANCRI
| Autor: | W. D. Cotton, Lee Anne Willson, Wesley A. Traub, M. G. Lacasse, S. Ragland, E. A. Pluzhnik, William C. Danchi |
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| Rok vydání: | 2009 |
| Předmět: |
Physics
Mira variable Infrared Astronomy Astronomy and Astrophysics Astrophysics::Cosmology and Extragalactic Astrophysics Astrophysics law.invention Stars Space and Planetary Science law Astrophysics::Solar and Stellar Astrophysics Asymptotic giant branch Astrophysics::Earth and Planetary Astrophysics Maser Variable star Infrared Optical Telescope Array Astrophysics::Galaxy Astrophysics Very Long Baseline Array |
| Zdroj: | The Astrophysical Journal Supplement Series. 185:574-585 |
| ISSN: | 1538-4365 0067-0049 |
| DOI: | 10.1088/0067-0049/185/2/574 |
| Popis: | This is the second paper in a series of multi-epoch observations of the SiO masers at 7 mm wavelength in several asymptotic giant branch stars from a sample of Mira variable stars showing evidence of asymmetric structure in the infrared. These stars have been observed interferometrically in the infrared by the Infrared Optical Telescope Array and with Very Long Baseline Array measurements of the SiO masers. In this paper, we present the observations of R Cancri (R Cnc). The systemic velocity of R Cnc is estimated to be 15.8 ± 0.2 km s–1. A comparison is made with the model calculations of Gray et al. which predict some but not all observed features. |
| Databáze: | OpenAIRE |
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