Back to Search
Start Over
DeSSpOt: an instrument for stellar spin orientation determination
- Publication Year :
- 2012
- Publisher :
- arXiv, 2012.
-
Abstract
- We designed and constructed a special instrument to enable the determination of the stellar's spin orientation. The Differential image rotator for Stellar Spin Orientation, DeSSpOt, allows the simultaneous observations of two anti-parallel orientations of the star on the spectrum. On a high resolution \'echelle spectrum, the stellar rotation causes a slight line tilt visible in the spatial direction which is comparable to a rotation curve. We developed a new method, which exploits the variations in these tilts, to estimate the absolute position angle of the rotation axis. The line tilt is retrieved by a spectro-astrometric extraction of the spectrum. In order to validate the method, we observed spectroscopic binaries with known orbital parameters. The determination of the orbital position angle is equivalent to the determination of the stellar position angle, but is easier to to detect. DeSSpOt was successfully implemented on the high resolution Coud\'e spectrograph of the Th\"uringer Landessternwarte Tautenburg. The observations of Capella led to the determination of the orbital position angle.<br />Comment: In-Press on the Proceedings of the SPIE Conference Astronomical Telescopes + instrumentation 2012, Amsterdam, paper #8446-149
- Subjects :
- Physics
Orbital elements
Stellar rotation
FOS: Physical sciences
Astrophysics
Rotation
Position angle
Tilt (optics)
Astrophysics - Solar and Stellar Astrophysics
Orientation (geometry)
Astrophysics::Solar and Stellar Astrophysics
Astrophysics::Earth and Planetary Astrophysics
Astrophysics - Instrumentation and Methods for Astrophysics
Spectrograph
Instrumentation and Methods for Astrophysics (astro-ph.IM)
Galaxy rotation curve
Astrophysics::Galaxy Astrophysics
Solar and Stellar Astrophysics (astro-ph.SR)
Subjects
Details
- Database :
- OpenAIRE
- Accession number :
- edsair.doi.dedup.....8e42b0f8cd95238917bb70f62f2d6740
- Full Text :
- https://doi.org/10.48550/arxiv.1208.2810