Astronomy and Astrophysics – Astronomy
Scientific paper
Jul 1994
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994aj....108..326h&link_type=abstract
The Astronomical Journal, vol. 108, no. 1, p. 326-336
Astronomy and Astrophysics
Astronomy
22
Astronomical Spectroscopy, F Stars, Main Sequence Stars, Michelson Interferometers, Stellar Motions, Stellar Rotation, Giant Stars, Histograms, Stellar Spectra
Scientific paper
Repeated measurements of the eleven FK5 stars selected by Shao et al. (AJ, 100, 1701 (1990)) were performed with the north-south and east-south astrometric baselines of the Mark III optical interferometer in order to estimate the accuracy of wide-angle astrometry. Even though the declination range of these stars is insufficient to determine absolute declinations, we were able to determine corrections to the FK5 positions at four epochs with an accuracy of about 13 milliarcseconds (mas) in declination and 23 mas in right ascension. Measurements at two different wavelengths were used to correct for refractive index fluctuations in the turbulent atmosphere. The pathlength difference between the two arms of the interferometer was monitored during the night with an internal white-light interferometer. The accuracy of the positions is limited by systematic errors due to unmonitored changes in the baseline coordinates and due to low-frequency water vapor fluctuations. However, these results demonstrate the potential of future optical interferometers for the measurement of stellar positions with mas accuracy.
Armstrong Thomas J.
Buscher David F.
Elias Nicholas M. II
Hummel Christian A.
Hutter Donald J.
No associations
LandOfFree
Four years of astrometric measurements with the Mark 3 optical interferometer does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Four years of astrometric measurements with the Mark 3 optical interferometer, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Four years of astrometric measurements with the Mark 3 optical interferometer will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1252653