Astronomy and Astrophysics – Astronomy
Scientific paper
Sep 1994
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994iraj...21..277a&link_type=abstract
Irish Astronomical Journal (ISSN 0021-1052), vol. 21, no. 3-4, p. 277-279
Astronomy and Astrophysics
Astronomy
Astronomical Photometry, Binary Stars, Emission Spectra, Extremely High Frequencies, Fast Fourier Transformations, Infrared Astronomy, Red Dwarf Stars, Stellar Oscillations, Data Processing, Data Reduction, H Alpha Line, Infrared Telescopes, Photometers, Temporal Resolution
Scientific paper
The red dwarf binary, Gliese 65AB (UV Cet) has been observed at subsecond time resolution in the K-band using the European Southern Observatory (ESO) 1 meter IR telescope with the fast photometer. Cumulative periodogram montages at one-third of a second resolution over about 2 hours were examined for transient periodicities in relation to the quiescent phase. A low-amplitude (less than 0.02 mag.) quasi-period of about 4.5 s (3.7-5.8 s) is suspected surviving several hundred cycles.
Andrews David A.
Panagi Peter M.
No associations
LandOfFree
Photometric oscillations and instrumental characteristics. 3: K-band cumulative periodogram montages and 4.5 second oscillations in UV CET 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 Photometric oscillations and instrumental characteristics. 3: K-band cumulative periodogram montages and 4.5 second oscillations in UV CET, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Photometric oscillations and instrumental characteristics. 3: K-band cumulative periodogram montages and 4.5 second oscillations in UV CET will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1790985