SIMBAD references

2005PASP..117..741S - Publ. Astron. Soc. Pac., 117, 741-744 (2005/July-0)

A spectroscopic study of HL Canis Majoris.

SHEETS H.A. and THORSTENSEN J.R.

Abstract (from CDS):

We present optical spectroscopy of the dwarf nova HL Canis Majoris over a span of 4 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 He I λ 5876 emission. We also present equivalent widths of the spectral features in outburst and in quiescence.

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Journal keyword(s): stars: dwarf novae - Stars: Individual: Constellation Name: HL Canis Majoris

Simbad objects: 2

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