Observations of RR Lyrae with the ANS satellite

Details Observations of RR Lyrae with the ANS satellite Observations of RR Lyrae with the ANS satellite

Dec 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982pasp...94..910b&link_type=abstract

Astronomical Society of the Pacific, Publications, vol. 94, Dec. 1982, p. 910-915. Research sponsored by the Koninklijke Nederla

Astronomy and Astrophysics

Astronomy

6

Astronomical Netherlands Satellite, Blue Stars, Giant Stars, Stellar Spectrophotometry, Ultraviolet Photometry, Variable Stars, Interstellar Extinction, Light Curve, Radiant Flux Density, Star Clusters, Stellar Temperature, Ultraviolet Astronomy

Scientific paper

Photometric observations of RR Lyr in the ultraviolet have been obtained using the Astronomical Netherlands Satellite. The observations are compared with theoretical light curves calculated using synthetic spectra and angular diameters determined as a function of phase for RR Lyr by Manduca et al. from photometry at longer wavelengths. A good agreement is found. A bump in the observed light curves in the phase range 0.6 to 0.8 supports the existence of a shock as predicted by Hutchinson, Hill, and Lillie.

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