Photometry of HR 5110 before, during, and after its radio outburst in June 1979

Details Photometry of HR 5110 before, during, and after its radio outburst in June 1979 Photometry of HR 5110 before, during, and after its radio outburst in June 1979

Jun 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980aj.....85..744b&link_type=abstract

Astronomical Journal, vol. 85, June 1980, p. 744-747.

Astronomy and Astrophysics

Astronomy

7

Binary Stars, Electrophotometry, Radio Bursts, Stellar Spectrophotometry, Data Processing, Stellar Magnitude

Scientific paper

Differential photoelectric photometry in V from seven different observatories is presented. No significant changes were seen in the V band coincident with the radio outburst. The mean light levels in 1978 and 1979 differ by only 0.0003 ± 0m.0003±0m.0016. Individual nights in 1979 fit the 1978 light curve within about ± 0m.01. From the reflection effect a more recent time of conjunction (cooler star in front) is derived: 2443639.52 ± 0d.05.

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