The angular diameter of R Doradus: a nearby Mira-like star
Abstract
We find the angular diameter of R Doradus to be 57+/-5mas, exceeding that of Betelgeuse and implying that R Dor is larger in apparent size than every star except the Sun. R Dor is shown to be closely related to the Mira variables. We estimate an effective temperature of 2740+/-190K, a distance of 61+/-7pc, a luminosity of 6500+/-1400 Lsolar and a radius of 370+/-50 Rsolar. The characteristics of R Dor are consistent with it being near the edge of a Mira instability strip. We detect non-zero closure phases from R Dor, indicating an asymmetric brightness distribution. We also observed W Hydrae, a small-amplitude Mira, for which we find an angular diameter of 44+/-4mas.
- Publication:
-
Monthly Notices of the Royal Astronomical Society
- Pub Date:
- April 1997
- DOI:
- 10.1093/mnras/286.4.957
- arXiv:
- arXiv:astro-ph/9701021
- Bibcode:
- 1997MNRAS.286..957B
- Keywords:
-
- TECHNIQUES: INTERFEROMETRIC;
- STARS: AGB AND POST-AGB;
- STARS: IMAGING;
- STARS: INDIVIDUAL: R DOR;
- STARS: INDIVIDUAL: ALPHA ORI;
- STARS: INDIVIDUAL: W HYA;
- Astrophysics
- E-Print:
- MNRAS (accepted)