Spectrophotometry of PG 1550 plus 191 at red wavelengths

Details Spectrophotometry of PG 1550 plus 191 at red wavelengths Spectrophotometry of PG 1550 plus 191 at red wavelengths

Jul 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982mnras.200p..23e&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 200, July 1982, p. 23P-26P. Research supported by the Consejo Nacional

Astronomy and Astrophysics

Astronomy

9

Stellar Spectra, Stellar Spectrophotometry, Variable Stars, Dwarf Stars, Light (Visible Radiation), M Stars, Titanium Oxides

Scientific paper

The spectrum of PG 1550+191, the new AM Herculis variable discovered by Stockman et al. (1981), has been observed from λλ 4400 to 8300 Å and shows titanium oxide bands. These bands can be associated with an M dwarf whose spectrum is superimposed on a continuum, together with an emission spectrum. An M type classification is in agreement with a Roche lobe-filling star at the orbital period discovered by Stockman et al. Lower and upper limits for the distance are 61 and 583 pc respectively.

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