Frequency analysis of photometric observations of HD 101158

Details Frequency analysis of photometric observations of HD 101158 Frequency analysis of photometric observations of HD 101158

Nov 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ap%26ss.127...27l&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 127, Nov. 1986, p. 27-32.

Astronomy and Astrophysics

Astrophysics

4

Cepheid Variables, Dwarf Stars, Electrophotometry, Spectrum Analysis, Stellar Spectrophotometry, Visible Spectrum, Fourier Analysis, Frequency Analyzers, Power Spectra

Scientific paper

Photoelectric observations of HD 101158 in visual light were obtained for six nights. A phase dispersion minimization method and Fourier analysis were used to derive a main frequency of 11.0877±0.0057 c/d or one of its aliases, 11.0648 and 11.1118 c/d. Some indications of multiplicity are presented. Because of the short period variability and the spectral type (F0 V), HD 101158 is found to be another Delta Scuti star.

Affiliated with

Also associated with

No associations

Rating

Frequency analysis of photometric observations of HD 101158 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 Frequency analysis of photometric observations of HD 101158, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Frequency analysis of photometric observations of HD 101158 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1148522