ar X iv : a st ro - p h / 05 06 06 8 v 1 2 J un 2 00 5 A Spectroscopic Study of HL Canis Majoris
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We present optical spectroscopy of the dwarf nova HL Canis Majoris over a span of four years. The observations were made during standstill, outburst, and quiescence. We determine an orbital period of 0.2167867 ± 0.0000017 days, based on radial velocities determined from Hα, Hβ, and HeI λ 5876 emission. We also present equivalent widths of the spectral features in outburst and in quiescence. Subject headings: stars: dwarf novae – stars: individual (HL CMa)
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تاریخ انتشار 2005