CoD-48 3636 deg - an apparently bright, low-luminosity, and high-temperature variable

Details CoD-48 3636 deg - an apparently bright, low-luminosity, and high-temperature variable CoD-48 3636 deg - an apparently bright, low-luminosity, and high-temperature variable

Mar 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984aj.....89..389e&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 89, March 1984, p. 389, 390.

Astronomy and Astrophysics

Astronomy

12

H Lines, Hot Stars, Stellar Spectra, Variable Stars, Emission Spectra, Radial Velocity, Stellar Luminosity, Visible Spectrum

Scientific paper

CoD -48°3636 has been found to be a low-luminosity and high-temperature variable with light variations on both short and long time scales and with radial velocity variations in the hydrogen emission lines with a period of 0.122 days. The star is probably a member of the Sirius Supercluster, giving Mv = +7 mag (π = 0arcsec.0305), and indicating similarity to the blue companions in such systems as RU Peg and AE Agr.

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