SiO Masers in Asymmetric Miras. II. R Cancri

Details SiO Masers in Asymmetric Miras. II. R Cancri SiO Masers in Asymmetric Miras. II. R Cancri

Dec 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009apjs..185..574c&link_type=abstract

The Astrophysical Journal Supplement, Volume 185, Issue 2, pp. 574-585 (2009).

Astronomy and Astrophysics

Astronomy

3

Radio Lines: Stars, Stars: Agb And Post-Agb, Stars: Atmospheres

Scientific paper

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.

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